diff --git a/docs/pyerrors/correlators.html b/docs/pyerrors/correlators.html index b96c4856..c6aff27c 100644 --- a/docs/pyerrors/correlators.html +++ b/docs/pyerrors/correlators.html @@ -61,6 +61,9 @@
Apply the gamma method to the content of the Corr.
+117 def gamma_method(self, **kwargs): +118 """Apply the gamma method to the content of the Corr.""" +119 for item in self.content: +120 if not (item is None): +121 if self.N == 1: +122 item[0].gamma_method(**kwargs) +123 else: +124 for i in range(self.N): +125 for j in range(self.N): +126 item[i, j].gamma_method(**kwargs) +
Apply the gamma method to the content of the Corr.
128 def projected(self, vector_l=None, vector_r=None, normalize=False): -129 """We need to project the Correlator with a Vector to get a single value at each timeslice. -130 -131 The method can use one or two vectors. -132 If two are specified it returns v1@G@v2 (the order might be very important.) -133 By default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to -134 """ -135 if self.N == 1: -136 raise Exception("Trying to project a Corr, that already has N=1.") -137 -138 if vector_l is None: -139 vector_l, vector_r = np.asarray([1.] + (self.N - 1) * [0.]), np.asarray([1.] + (self.N - 1) * [0.]) -140 elif (vector_r is None): -141 vector_r = vector_l -142 if isinstance(vector_l, list) and not isinstance(vector_r, list): -143 if len(vector_l) != self.T: -144 raise Exception("Length of vector list must be equal to T") -145 vector_r = [vector_r] * self.T -146 if isinstance(vector_r, list) and not isinstance(vector_l, list): -147 if len(vector_r) != self.T: -148 raise Exception("Length of vector list must be equal to T") -149 vector_l = [vector_l] * self.T -150 -151 if not isinstance(vector_l, list): -152 if not vector_l.shape == vector_r.shape == (self.N,): -153 raise Exception("Vectors are of wrong shape!") -154 if normalize: -155 vector_l, vector_r = vector_l / np.sqrt((vector_l @ vector_l)), vector_r / np.sqrt(vector_r @ vector_r) -156 newcontent = [None if _check_for_none(self, item) else np.asarray([vector_l.T @ item @ vector_r]) for item in self.content] -157 -158 else: -159 # There are no checks here yet. There are so many possible scenarios, where this can go wrong. -160 if normalize: -161 for t in range(self.T): -162 vector_l[t], vector_r[t] = vector_l[t] / np.sqrt((vector_l[t] @ vector_l[t])), vector_r[t] / np.sqrt(vector_r[t] @ vector_r[t]) -163 -164 newcontent = [None if (_check_for_none(self, self.content[t]) or vector_l[t] is None or vector_r[t] is None) else np.asarray([vector_l[t].T @ self.content[t] @ vector_r[t]]) for t in range(self.T)] -165 return Corr(newcontent) +@@ -3019,20 +3055,20 @@ By default it will return the lowest source, which usually means unsmeared-unsme130 def projected(self, vector_l=None, vector_r=None, normalize=False): +131 """We need to project the Correlator with a Vector to get a single value at each timeslice. +132 +133 The method can use one or two vectors. +134 If two are specified it returns v1@G@v2 (the order might be very important.) +135 By default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to +136 """ +137 if self.N == 1: +138 raise Exception("Trying to project a Corr, that already has N=1.") +139 +140 if vector_l is None: +141 vector_l, vector_r = np.asarray([1.] + (self.N - 1) * [0.]), np.asarray([1.] + (self.N - 1) * [0.]) +142 elif (vector_r is None): +143 vector_r = vector_l +144 if isinstance(vector_l, list) and not isinstance(vector_r, list): +145 if len(vector_l) != self.T: +146 raise Exception("Length of vector list must be equal to T") +147 vector_r = [vector_r] * self.T +148 if isinstance(vector_r, list) and not isinstance(vector_l, list): +149 if len(vector_r) != self.T: +150 raise Exception("Length of vector list must be equal to T") +151 vector_l = [vector_l] * self.T +152 +153 if not isinstance(vector_l, list): +154 if not vector_l.shape == vector_r.shape == (self.N,): +155 raise Exception("Vectors are of wrong shape!") +156 if normalize: +157 vector_l, vector_r = vector_l / np.sqrt((vector_l @ vector_l)), vector_r / np.sqrt(vector_r @ vector_r) +158 newcontent = [None if _check_for_none(self, item) else np.asarray([vector_l.T @ item @ vector_r]) for item in self.content] +159 +160 else: +161 # There are no checks here yet. There are so many possible scenarios, where this can go wrong. +162 if normalize: +163 for t in range(self.T): +164 vector_l[t], vector_r[t] = vector_l[t] / np.sqrt((vector_l[t] @ vector_l[t])), vector_r[t] / np.sqrt(vector_r[t] @ vector_r[t]) +165 +166 newcontent = [None if (_check_for_none(self, self.content[t]) or vector_l[t] is None or vector_r[t] is None) else np.asarray([vector_l[t].T @ self.content[t] @ vector_r[t]]) for t in range(self.T)] +167 return Corr(newcontent)
167 def item(self, i, j): -168 """Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice. -169 -170 Parameters -171 ---------- -172 i : int -173 First index to be picked. -174 j : int -175 Second index to be picked. -176 """ -177 if self.N == 1: -178 raise Exception("Trying to pick item from projected Corr") -179 newcontent = [None if (item is None) else item[i, j] for item in self.content] -180 return Corr(newcontent) +@@ -3061,19 +3097,19 @@ Second index to be picked.169 def item(self, i, j): +170 """Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice. +171 +172 Parameters +173 ---------- +174 i : int +175 First index to be picked. +176 j : int +177 Second index to be picked. +178 """ +179 if self.N == 1: +180 raise Exception("Trying to pick item from projected Corr") +181 newcontent = [None if (item is None) else item[i, j] for item in self.content] +182 return Corr(newcontent)
182 def plottable(self): -183 """Outputs the correlator in a plotable format. -184 -185 Outputs three lists containing the timeslice index, the value on each -186 timeslice and the error on each timeslice. -187 """ -188 if self.N != 1: -189 raise Exception("Can only make Corr[N=1] plottable") -190 x_list = [x for x in range(self.T) if not self.content[x] is None] -191 y_list = [y[0].value for y in self.content if y is not None] -192 y_err_list = [y[0].dvalue for y in self.content if y is not None] -193 -194 return x_list, y_list, y_err_list +@@ -3096,25 +3132,25 @@ timeslice and the error on each timeslice.184 def plottable(self): +185 """Outputs the correlator in a plotable format. +186 +187 Outputs three lists containing the timeslice index, the value on each +188 timeslice and the error on each timeslice. +189 """ +190 if self.N != 1: +191 raise Exception("Can only make Corr[N=1] plottable") +192 x_list = [x for x in range(self.T) if not self.content[x] is None] +193 y_list = [y[0].value for y in self.content if y is not None] +194 y_err_list = [y[0].dvalue for y in self.content if y is not None] +195 +196 return x_list, y_list, y_err_list
196 def symmetric(self): -197 """ Symmetrize the correlator around x0=0.""" -198 if self.N != 1: -199 raise Exception('symmetric cannot be safely applied to multi-dimensional correlators.') -200 if self.T % 2 != 0: -201 raise Exception("Can not symmetrize odd T") -202 -203 if np.argmax(np.abs(self.content)) != 0: -204 warnings.warn("Correlator does not seem to be symmetric around x0=0.", RuntimeWarning) -205 -206 newcontent = [self.content[0]] -207 for t in range(1, self.T): -208 if (self.content[t] is None) or (self.content[self.T - t] is None): -209 newcontent.append(None) -210 else: -211 newcontent.append(0.5 * (self.content[t] + self.content[self.T - t])) -212 if (all([x is None for x in newcontent])): -213 raise Exception("Corr could not be symmetrized: No redundant values") -214 return Corr(newcontent, prange=self.prange) +@@ -3134,27 +3170,27 @@ timeslice and the error on each timeslice.198 def symmetric(self): +199 """ Symmetrize the correlator around x0=0.""" +200 if self.N != 1: +201 raise Exception('symmetric cannot be safely applied to multi-dimensional correlators.') +202 if self.T % 2 != 0: +203 raise Exception("Can not symmetrize odd T") +204 +205 if np.argmax(np.abs(self.content)) != 0: +206 warnings.warn("Correlator does not seem to be symmetric around x0=0.", RuntimeWarning) +207 +208 newcontent = [self.content[0]] +209 for t in range(1, self.T): +210 if (self.content[t] is None) or (self.content[self.T - t] is None): +211 newcontent.append(None) +212 else: +213 newcontent.append(0.5 * (self.content[t] + self.content[self.T - t])) +214 if (all([x is None for x in newcontent])): +215 raise Exception("Corr could not be symmetrized: No redundant values") +216 return Corr(newcontent, prange=self.prange)
216 def anti_symmetric(self): -217 """Anti-symmetrize the correlator around x0=0.""" -218 if self.N != 1: -219 raise Exception('anti_symmetric cannot be safely applied to multi-dimensional correlators.') -220 if self.T % 2 != 0: -221 raise Exception("Can not symmetrize odd T") -222 -223 test = 1 * self -224 test.gamma_method() -225 if not all([o.is_zero_within_error(3) for o in test.content[0]]): -226 warnings.warn("Correlator does not seem to be anti-symmetric around x0=0.", RuntimeWarning) -227 -228 newcontent = [self.content[0]] -229 for t in range(1, self.T): -230 if (self.content[t] is None) or (self.content[self.T - t] is None): -231 newcontent.append(None) -232 else: -233 newcontent.append(0.5 * (self.content[t] - self.content[self.T - t])) -234 if (all([x is None for x in newcontent])): -235 raise Exception("Corr could not be symmetrized: No redundant values") -236 return Corr(newcontent, prange=self.prange) +@@ -3174,20 +3210,20 @@ timeslice and the error on each timeslice.218 def anti_symmetric(self): +219 """Anti-symmetrize the correlator around x0=0.""" +220 if self.N != 1: +221 raise Exception('anti_symmetric cannot be safely applied to multi-dimensional correlators.') +222 if self.T % 2 != 0: +223 raise Exception("Can not symmetrize odd T") +224 +225 test = 1 * self +226 test.gamma_method() +227 if not all([o.is_zero_within_error(3) for o in test.content[0]]): +228 warnings.warn("Correlator does not seem to be anti-symmetric around x0=0.", RuntimeWarning) +229 +230 newcontent = [self.content[0]] +231 for t in range(1, self.T): +232 if (self.content[t] is None) or (self.content[self.T - t] is None): +233 newcontent.append(None) +234 else: +235 newcontent.append(0.5 * (self.content[t] - self.content[self.T - t])) +236 if (all([x is None for x in newcontent])): +237 raise Exception("Corr could not be symmetrized: No redundant values") +238 return Corr(newcontent, prange=self.prange)
238 def is_matrix_symmetric(self): -239 """Checks whether a correlator matrices is symmetric on every timeslice.""" -240 if self.N == 1: -241 raise Exception("Only works for correlator matrices.") -242 for t in range(self.T): -243 if self[t] is None: -244 continue -245 for i in range(self.N): -246 for j in range(i + 1, self.N): -247 if self[t][i, j] is self[t][j, i]: -248 continue -249 if hash(self[t][i, j]) != hash(self[t][j, i]): -250 return False -251 return True +@@ -3207,15 +3243,15 @@ timeslice and the error on each timeslice.240 def is_matrix_symmetric(self): +241 """Checks whether a correlator matrices is symmetric on every timeslice.""" +242 if self.N == 1: +243 raise Exception("Only works for correlator matrices.") +244 for t in range(self.T): +245 if self[t] is None: +246 continue +247 for i in range(self.N): +248 for j in range(i + 1, self.N): +249 if self[t][i, j] is self[t][j, i]: +250 continue +251 if hash(self[t][i, j]) != hash(self[t][j, i]): +252 return False +253 return True
253 def matrix_symmetric(self): -254 """Symmetrizes the correlator matrices on every timeslice.""" -255 if self.N == 1: -256 raise Exception("Trying to symmetrize a correlator matrix, that already has N=1.") -257 if self.is_matrix_symmetric(): -258 return 1.0 * self -259 else: -260 transposed = [None if _check_for_none(self, G) else G.T for G in self.content] -261 return 0.5 * (Corr(transposed) + self) +@@ -3235,84 +3271,84 @@ timeslice and the error on each timeslice.255 def matrix_symmetric(self): +256 """Symmetrizes the correlator matrices on every timeslice.""" +257 if self.N == 1: +258 raise Exception("Trying to symmetrize a correlator matrix, that already has N=1.") +259 if self.is_matrix_symmetric(): +260 return 1.0 * self +261 else: +262 transposed = [None if _check_for_none(self, G) else G.T for G in self.content] +263 return 0.5 * (Corr(transposed) + self)
263 def GEVP(self, t0, ts=None, sort="Eigenvalue", **kwargs): -264 r'''Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors. -265 -266 The eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the -267 largest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing -268 ```python -269 C.GEVP(t0=2)[0] # Ground state vector(s) -270 C.GEVP(t0=2)[:3] # Vectors for the lowest three states -271 ``` -272 -273 Parameters -274 ---------- -275 t0 : int -276 The time t0 for the right hand side of the GEVP according to $G(t)v_i=\lambda_i G(t_0)v_i$ -277 ts : int -278 fixed time $G(t_s)v_i=\lambda_i G(t_0)v_i$ if sort=None. -279 If sort="Eigenvector" it gives a reference point for the sorting method. -280 sort : string -281 If this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned. -282 - "Eigenvalue": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice. -283 - "Eigenvector": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state. -284 The reference state is identified by its eigenvalue at $t=t_s$. -285 -286 Other Parameters -287 ---------------- -288 state : int -289 Returns only the vector(s) for a specified state. The lowest state is zero. -290 ''' -291 -292 if self.N == 1: -293 raise Exception("GEVP methods only works on correlator matrices and not single correlators.") -294 if ts is not None: -295 if (ts <= t0): -296 raise Exception("ts has to be larger than t0.") -297 -298 if "sorted_list" in kwargs: -299 warnings.warn("Argument 'sorted_list' is deprecated, use 'sort' instead.", DeprecationWarning) -300 sort = kwargs.get("sorted_list") -301 -302 if self.is_matrix_symmetric(): -303 symmetric_corr = self -304 else: -305 symmetric_corr = self.matrix_symmetric() -306 -307 G0 = np.vectorize(lambda x: x.value)(symmetric_corr[t0]) -308 np.linalg.cholesky(G0) # Check if matrix G0 is positive-semidefinite. -309 -310 if sort is None: -311 if (ts is None): -312 raise Exception("ts is required if sort=None.") -313 if (self.content[t0] is None) or (self.content[ts] is None): -314 raise Exception("Corr not defined at t0/ts.") -315 Gt = np.vectorize(lambda x: x.value)(symmetric_corr[ts]) -316 reordered_vecs = _GEVP_solver(Gt, G0) -317 -318 elif sort in ["Eigenvalue", "Eigenvector"]: -319 if sort == "Eigenvalue" and ts is not None: -320 warnings.warn("ts has no effect when sorting by eigenvalue is chosen.", RuntimeWarning) -321 all_vecs = [None] * (t0 + 1) -322 for t in range(t0 + 1, self.T): -323 try: -324 Gt = np.vectorize(lambda x: x.value)(symmetric_corr[t]) -325 all_vecs.append(_GEVP_solver(Gt, G0)) -326 except Exception: -327 all_vecs.append(None) -328 if sort == "Eigenvector": -329 if ts is None: -330 raise Exception("ts is required for the Eigenvector sorting method.") -331 all_vecs = _sort_vectors(all_vecs, ts) -332 -333 reordered_vecs = [[v[s] if v is not None else None for v in all_vecs] for s in range(self.N)] -334 else: -335 raise Exception("Unkown value for 'sort'.") -336 -337 if "state" in kwargs: -338 return reordered_vecs[kwargs.get("state")] -339 else: -340 return reordered_vecs +@@ -3365,18 +3401,18 @@ Returns only the vector(s) for a specified state. The lowest state is zero.265 def GEVP(self, t0, ts=None, sort="Eigenvalue", **kwargs): +266 r'''Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors. +267 +268 The eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the +269 largest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing +270 ```python +271 C.GEVP(t0=2)[0] # Ground state vector(s) +272 C.GEVP(t0=2)[:3] # Vectors for the lowest three states +273 ``` +274 +275 Parameters +276 ---------- +277 t0 : int +278 The time t0 for the right hand side of the GEVP according to $G(t)v_i=\lambda_i G(t_0)v_i$ +279 ts : int +280 fixed time $G(t_s)v_i=\lambda_i G(t_0)v_i$ if sort=None. +281 If sort="Eigenvector" it gives a reference point for the sorting method. +282 sort : string +283 If this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned. +284 - "Eigenvalue": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice. +285 - "Eigenvector": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state. +286 The reference state is identified by its eigenvalue at $t=t_s$. +287 +288 Other Parameters +289 ---------------- +290 state : int +291 Returns only the vector(s) for a specified state. The lowest state is zero. +292 ''' +293 +294 if self.N == 1: +295 raise Exception("GEVP methods only works on correlator matrices and not single correlators.") +296 if ts is not None: +297 if (ts <= t0): +298 raise Exception("ts has to be larger than t0.") +299 +300 if "sorted_list" in kwargs: +301 warnings.warn("Argument 'sorted_list' is deprecated, use 'sort' instead.", DeprecationWarning) +302 sort = kwargs.get("sorted_list") +303 +304 if self.is_matrix_symmetric(): +305 symmetric_corr = self +306 else: +307 symmetric_corr = self.matrix_symmetric() +308 +309 G0 = np.vectorize(lambda x: x.value)(symmetric_corr[t0]) +310 np.linalg.cholesky(G0) # Check if matrix G0 is positive-semidefinite. +311 +312 if sort is None: +313 if (ts is None): +314 raise Exception("ts is required if sort=None.") +315 if (self.content[t0] is None) or (self.content[ts] is None): +316 raise Exception("Corr not defined at t0/ts.") +317 Gt = np.vectorize(lambda x: x.value)(symmetric_corr[ts]) +318 reordered_vecs = _GEVP_solver(Gt, G0) +319 +320 elif sort in ["Eigenvalue", "Eigenvector"]: +321 if sort == "Eigenvalue" and ts is not None: +322 warnings.warn("ts has no effect when sorting by eigenvalue is chosen.", RuntimeWarning) +323 all_vecs = [None] * (t0 + 1) +324 for t in range(t0 + 1, self.T): +325 try: +326 Gt = np.vectorize(lambda x: x.value)(symmetric_corr[t]) +327 all_vecs.append(_GEVP_solver(Gt, G0)) +328 except Exception: +329 all_vecs.append(None) +330 if sort == "Eigenvector": +331 if ts is None: +332 raise Exception("ts is required for the Eigenvector sorting method.") +333 all_vecs = _sort_vectors(all_vecs, ts) +334 +335 reordered_vecs = [[v[s] if v is not None else None for v in all_vecs] for s in range(self.N)] +336 else: +337 raise Exception("Unkown value for 'sort'.") +338 +339 if "state" in kwargs: +340 return reordered_vecs[kwargs.get("state")] +341 else: +342 return reordered_vecs
342 def Eigenvalue(self, t0, ts=None, state=0, sort="Eigenvalue"): -343 """Determines the eigenvalue of the GEVP by solving and projecting the correlator -344 -345 Parameters -346 ---------- -347 state : int -348 The state one is interested in ordered by energy. The lowest state is zero. -349 -350 All other parameters are identical to the ones of Corr.GEVP. -351 """ -352 vec = self.GEVP(t0, ts=ts, sort=sort)[state] -353 return self.projected(vec) +@@ -3404,46 +3440,46 @@ The state one is interested in ordered by energy. The lowest state is zero.344 def Eigenvalue(self, t0, ts=None, state=0, sort="Eigenvalue"): +345 """Determines the eigenvalue of the GEVP by solving and projecting the correlator +346 +347 Parameters +348 ---------- +349 state : int +350 The state one is interested in ordered by energy. The lowest state is zero. +351 +352 All other parameters are identical to the ones of Corr.GEVP. +353 """ +354 vec = self.GEVP(t0, ts=ts, sort=sort)[state] +355 return self.projected(vec)
355 def Hankel(self, N, periodic=False): -356 """Constructs an NxN Hankel matrix -357 -358 C(t) c(t+1) ... c(t+n-1) -359 C(t+1) c(t+2) ... c(t+n) -360 ................. -361 C(t+(n-1)) c(t+n) ... c(t+2(n-1)) -362 -363 Parameters -364 ---------- -365 N : int -366 Dimension of the Hankel matrix -367 periodic : bool, optional -368 determines whether the matrix is extended periodically -369 """ -370 -371 if self.N != 1: -372 raise Exception("Multi-operator Prony not implemented!") -373 -374 array = np.empty([N, N], dtype="object") -375 new_content = [] -376 for t in range(self.T): -377 new_content.append(array.copy()) -378 -379 def wrap(i): -380 while i >= self.T: -381 i -= self.T -382 return i -383 -384 for t in range(self.T): -385 for i in range(N): -386 for j in range(N): -387 if periodic: -388 new_content[t][i, j] = self.content[wrap(t + i + j)][0] -389 elif (t + i + j) >= self.T: -390 new_content[t] = None -391 else: -392 new_content[t][i, j] = self.content[t + i + j][0] -393 -394 return Corr(new_content) +@@ -3477,15 +3513,15 @@ determines whether the matrix is extended periodically357 def Hankel(self, N, periodic=False): +358 """Constructs an NxN Hankel matrix +359 +360 C(t) c(t+1) ... c(t+n-1) +361 C(t+1) c(t+2) ... c(t+n) +362 ................. +363 C(t+(n-1)) c(t+n) ... c(t+2(n-1)) +364 +365 Parameters +366 ---------- +367 N : int +368 Dimension of the Hankel matrix +369 periodic : bool, optional +370 determines whether the matrix is extended periodically +371 """ +372 +373 if self.N != 1: +374 raise Exception("Multi-operator Prony not implemented!") +375 +376 array = np.empty([N, N], dtype="object") +377 new_content = [] +378 for t in range(self.T): +379 new_content.append(array.copy()) +380 +381 def wrap(i): +382 while i >= self.T: +383 i -= self.T +384 return i +385 +386 for t in range(self.T): +387 for i in range(N): +388 for j in range(N): +389 if periodic: +390 new_content[t][i, j] = self.content[wrap(t + i + j)][0] +391 elif (t + i + j) >= self.T: +392 new_content[t] = None +393 else: +394 new_content[t][i, j] = self.content[t + i + j][0] +395 +396 return Corr(new_content)
396 def roll(self, dt): -397 """Periodically shift the correlator by dt timeslices -398 -399 Parameters -400 ---------- -401 dt : int -402 number of timeslices -403 """ -404 return Corr(list(np.roll(np.array(self.content, dtype=object), dt))) + @@ -3512,9 +3548,9 @@ number of timeslices
406 def reverse(self): -407 """Reverse the time ordering of the Corr""" -408 return Corr(self.content[:: -1]) + @@ -3534,23 +3570,23 @@ number of timeslices
410 def thin(self, spacing=2, offset=0): -411 """Thin out a correlator to suppress correlations -412 -413 Parameters -414 ---------- -415 spacing : int -416 Keep only every 'spacing'th entry of the correlator -417 offset : int -418 Offset the equal spacing -419 """ -420 new_content = [] -421 for t in range(self.T): -422 if (offset + t) % spacing != 0: -423 new_content.append(None) -424 else: -425 new_content.append(self.content[t]) -426 return Corr(new_content) +@@ -3579,34 +3615,34 @@ Offset the equal spacing412 def thin(self, spacing=2, offset=0): +413 """Thin out a correlator to suppress correlations +414 +415 Parameters +416 ---------- +417 spacing : int +418 Keep only every 'spacing'th entry of the correlator +419 offset : int +420 Offset the equal spacing +421 """ +422 new_content = [] +423 for t in range(self.T): +424 if (offset + t) % spacing != 0: +425 new_content.append(None) +426 else: +427 new_content.append(self.content[t]) +428 return Corr(new_content)
428 def correlate(self, partner): -429 """Correlate the correlator with another correlator or Obs -430 -431 Parameters -432 ---------- -433 partner : Obs or Corr -434 partner to correlate the correlator with. -435 Can either be an Obs which is correlated with all entries of the -436 correlator or a Corr of same length. -437 """ -438 if self.N != 1: -439 raise Exception("Only one-dimensional correlators can be safely correlated.") -440 new_content = [] -441 for x0, t_slice in enumerate(self.content): -442 if _check_for_none(self, t_slice): -443 new_content.append(None) -444 else: -445 if isinstance(partner, Corr): -446 if _check_for_none(partner, partner.content[x0]): -447 new_content.append(None) -448 else: -449 new_content.append(np.array([correlate(o, partner.content[x0][0]) for o in t_slice])) -450 elif isinstance(partner, Obs): # Should this include CObs? -451 new_content.append(np.array([correlate(o, partner) for o in t_slice])) -452 else: -453 raise Exception("Can only correlate with an Obs or a Corr.") -454 -455 return Corr(new_content) +@@ -3635,28 +3671,28 @@ correlator or a Corr of same length.430 def correlate(self, partner): +431 """Correlate the correlator with another correlator or Obs +432 +433 Parameters +434 ---------- +435 partner : Obs or Corr +436 partner to correlate the correlator with. +437 Can either be an Obs which is correlated with all entries of the +438 correlator or a Corr of same length. +439 """ +440 if self.N != 1: +441 raise Exception("Only one-dimensional correlators can be safely correlated.") +442 new_content = [] +443 for x0, t_slice in enumerate(self.content): +444 if _check_for_none(self, t_slice): +445 new_content.append(None) +446 else: +447 if isinstance(partner, Corr): +448 if _check_for_none(partner, partner.content[x0]): +449 new_content.append(None) +450 else: +451 new_content.append(np.array([correlate(o, partner.content[x0][0]) for o in t_slice])) +452 elif isinstance(partner, Obs): # Should this include CObs? +453 new_content.append(np.array([correlate(o, partner) for o in t_slice])) +454 else: +455 raise Exception("Can only correlate with an Obs or a Corr.") +456 +457 return Corr(new_content)
457 def reweight(self, weight, **kwargs): -458 """Reweight the correlator. -459 -460 Parameters -461 ---------- -462 weight : Obs -463 Reweighting factor. An Observable that has to be defined on a superset of the -464 configurations in obs[i].idl for all i. -465 all_configs : bool -466 if True, the reweighted observables are normalized by the average of -467 the reweighting factor on all configurations in weight.idl and not -468 on the configurations in obs[i].idl. -469 """ -470 if self.N != 1: -471 raise Exception("Reweighting only implemented for one-dimensional correlators.") -472 new_content = [] -473 for t_slice in self.content: -474 if _check_for_none(self, t_slice): -475 new_content.append(None) -476 else: -477 new_content.append(np.array(reweight(weight, t_slice, **kwargs))) -478 return Corr(new_content) +@@ -3688,35 +3724,35 @@ on the configurations in obs[i].idl.459 def reweight(self, weight, **kwargs): +460 """Reweight the correlator. +461 +462 Parameters +463 ---------- +464 weight : Obs +465 Reweighting factor. An Observable that has to be defined on a superset of the +466 configurations in obs[i].idl for all i. +467 all_configs : bool +468 if True, the reweighted observables are normalized by the average of +469 the reweighting factor on all configurations in weight.idl and not +470 on the configurations in obs[i].idl. +471 """ +472 if self.N != 1: +473 raise Exception("Reweighting only implemented for one-dimensional correlators.") +474 new_content = [] +475 for t_slice in self.content: +476 if _check_for_none(self, t_slice): +477 new_content.append(None) +478 else: +479 new_content.append(np.array(reweight(weight, t_slice, **kwargs))) +480 return Corr(new_content)
480 def T_symmetry(self, partner, parity=+1): -481 """Return the time symmetry average of the correlator and its partner -482 -483 Parameters -484 ---------- -485 partner : Corr -486 Time symmetry partner of the Corr -487 partity : int -488 Parity quantum number of the correlator, can be +1 or -1 -489 """ -490 if self.N != 1: -491 raise Exception("T_symmetry only implemented for one-dimensional correlators.") -492 if not isinstance(partner, Corr): -493 raise Exception("T partner has to be a Corr object.") -494 if parity not in [+1, -1]: -495 raise Exception("Parity has to be +1 or -1.") -496 T_partner = parity * partner.reverse() -497 -498 t_slices = [] -499 test = (self - T_partner) -500 test.gamma_method() -501 for x0, t_slice in enumerate(test.content): -502 if t_slice is not None: -503 if not t_slice[0].is_zero_within_error(5): -504 t_slices.append(x0) -505 if t_slices: -506 warnings.warn("T symmetry partners do not agree within 5 sigma on time slices " + str(t_slices) + ".", RuntimeWarning) -507 -508 return (self + T_partner) / 2 +@@ -3745,70 +3781,70 @@ Parity quantum number of the correlator, can be +1 or -1482 def T_symmetry(self, partner, parity=+1): +483 """Return the time symmetry average of the correlator and its partner +484 +485 Parameters +486 ---------- +487 partner : Corr +488 Time symmetry partner of the Corr +489 partity : int +490 Parity quantum number of the correlator, can be +1 or -1 +491 """ +492 if self.N != 1: +493 raise Exception("T_symmetry only implemented for one-dimensional correlators.") +494 if not isinstance(partner, Corr): +495 raise Exception("T partner has to be a Corr object.") +496 if parity not in [+1, -1]: +497 raise Exception("Parity has to be +1 or -1.") +498 T_partner = parity * partner.reverse() +499 +500 t_slices = [] +501 test = (self - T_partner) +502 test.gamma_method() +503 for x0, t_slice in enumerate(test.content): +504 if t_slice is not None: +505 if not t_slice[0].is_zero_within_error(5): +506 t_slices.append(x0) +507 if t_slices: +508 warnings.warn("T symmetry partners do not agree within 5 sigma on time slices " + str(t_slices) + ".", RuntimeWarning) +509 +510 return (self + T_partner) / 2
510 def deriv(self, variant="symmetric"): -511 """Return the first derivative of the correlator with respect to x0. -512 -513 Parameters -514 ---------- -515 variant : str -516 decides which definition of the finite differences derivative is used. -517 Available choice: symmetric, forward, backward, improved, log, default: symmetric -518 """ -519 if self.N != 1: -520 raise Exception("deriv only implemented for one-dimensional correlators.") -521 if variant == "symmetric": -522 newcontent = [] -523 for t in range(1, self.T - 1): -524 if (self.content[t - 1] is None) or (self.content[t + 1] is None): -525 newcontent.append(None) -526 else: -527 newcontent.append(0.5 * (self.content[t + 1] - self.content[t - 1])) -528 if (all([x is None for x in newcontent])): -529 raise Exception('Derivative is undefined at all timeslices') -530 return Corr(newcontent, padding=[1, 1]) -531 elif variant == "forward": -532 newcontent = [] -533 for t in range(self.T - 1): -534 if (self.content[t] is None) or (self.content[t + 1] is None): -535 newcontent.append(None) -536 else: -537 newcontent.append(self.content[t + 1] - self.content[t]) -538 if (all([x is None for x in newcontent])): -539 raise Exception("Derivative is undefined at all timeslices") -540 return Corr(newcontent, padding=[0, 1]) -541 elif variant == "backward": -542 newcontent = [] -543 for t in range(1, self.T): -544 if (self.content[t - 1] is None) or (self.content[t] is None): -545 newcontent.append(None) -546 else: -547 newcontent.append(self.content[t] - self.content[t - 1]) -548 if (all([x is None for x in newcontent])): -549 raise Exception("Derivative is undefined at all timeslices") -550 return Corr(newcontent, padding=[1, 0]) -551 elif variant == "improved": -552 newcontent = [] -553 for t in range(2, self.T - 2): -554 if (self.content[t - 2] is None) or (self.content[t - 1] is None) or (self.content[t + 1] is None) or (self.content[t + 2] is None): -555 newcontent.append(None) -556 else: -557 newcontent.append((1 / 12) * (self.content[t - 2] - 8 * self.content[t - 1] + 8 * self.content[t + 1] - self.content[t + 2])) -558 if (all([x is None for x in newcontent])): -559 raise Exception('Derivative is undefined at all timeslices') -560 return Corr(newcontent, padding=[2, 2]) -561 elif variant == 'log': -562 newcontent = [] -563 for t in range(self.T): -564 if (self.content[t] is None) or (self.content[t] <= 0): -565 newcontent.append(None) -566 else: -567 newcontent.append(np.log(self.content[t])) -568 if (all([x is None for x in newcontent])): -569 raise Exception("Log is undefined at all timeslices") -570 logcorr = Corr(newcontent) -571 return self * logcorr.deriv('symmetric') -572 else: -573 raise Exception("Unknown variant.") +@@ -3836,50 +3872,50 @@ Available choice: symmetric, forward, backward, improved, log, default: symmetri512 def deriv(self, variant="symmetric"): +513 """Return the first derivative of the correlator with respect to x0. +514 +515 Parameters +516 ---------- +517 variant : str +518 decides which definition of the finite differences derivative is used. +519 Available choice: symmetric, forward, backward, improved, log, default: symmetric +520 """ +521 if self.N != 1: +522 raise Exception("deriv only implemented for one-dimensional correlators.") +523 if variant == "symmetric": +524 newcontent = [] +525 for t in range(1, self.T - 1): +526 if (self.content[t - 1] is None) or (self.content[t + 1] is None): +527 newcontent.append(None) +528 else: +529 newcontent.append(0.5 * (self.content[t + 1] - self.content[t - 1])) +530 if (all([x is None for x in newcontent])): +531 raise Exception('Derivative is undefined at all timeslices') +532 return Corr(newcontent, padding=[1, 1]) +533 elif variant == "forward": +534 newcontent = [] +535 for t in range(self.T - 1): +536 if (self.content[t] is None) or (self.content[t + 1] is None): +537 newcontent.append(None) +538 else: +539 newcontent.append(self.content[t + 1] - self.content[t]) +540 if (all([x is None for x in newcontent])): +541 raise Exception("Derivative is undefined at all timeslices") +542 return Corr(newcontent, padding=[0, 1]) +543 elif variant == "backward": +544 newcontent = [] +545 for t in range(1, self.T): +546 if (self.content[t - 1] is None) or (self.content[t] is None): +547 newcontent.append(None) +548 else: +549 newcontent.append(self.content[t] - self.content[t - 1]) +550 if (all([x is None for x in newcontent])): +551 raise Exception("Derivative is undefined at all timeslices") +552 return Corr(newcontent, padding=[1, 0]) +553 elif variant == "improved": +554 newcontent = [] +555 for t in range(2, self.T - 2): +556 if (self.content[t - 2] is None) or (self.content[t - 1] is None) or (self.content[t + 1] is None) or (self.content[t + 2] is None): +557 newcontent.append(None) +558 else: +559 newcontent.append((1 / 12) * (self.content[t - 2] - 8 * self.content[t - 1] + 8 * self.content[t + 1] - self.content[t + 2])) +560 if (all([x is None for x in newcontent])): +561 raise Exception('Derivative is undefined at all timeslices') +562 return Corr(newcontent, padding=[2, 2]) +563 elif variant == 'log': +564 newcontent = [] +565 for t in range(self.T): +566 if (self.content[t] is None) or (self.content[t] <= 0): +567 newcontent.append(None) +568 else: +569 newcontent.append(np.log(self.content[t])) +570 if (all([x is None for x in newcontent])): +571 raise Exception("Log is undefined at all timeslices") +572 logcorr = Corr(newcontent) +573 return self * logcorr.deriv('symmetric') +574 else: +575 raise Exception("Unknown variant.")
575 def second_deriv(self, variant="symmetric"): -576 """Return the second derivative of the correlator with respect to x0. -577 -578 Parameters -579 ---------- -580 variant : str -581 decides which definition of the finite differences derivative is used. -582 Available choice: symmetric, improved, log, default: symmetric -583 """ -584 if self.N != 1: -585 raise Exception("second_deriv only implemented for one-dimensional correlators.") -586 if variant == "symmetric": -587 newcontent = [] -588 for t in range(1, self.T - 1): -589 if (self.content[t - 1] is None) or (self.content[t + 1] is None): -590 newcontent.append(None) -591 else: -592 newcontent.append((self.content[t + 1] - 2 * self.content[t] + self.content[t - 1])) -593 if (all([x is None for x in newcontent])): -594 raise Exception("Derivative is undefined at all timeslices") -595 return Corr(newcontent, padding=[1, 1]) -596 elif variant == "improved": -597 newcontent = [] -598 for t in range(2, self.T - 2): -599 if (self.content[t - 2] is None) or (self.content[t - 1] is None) or (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t + 2] is None): -600 newcontent.append(None) -601 else: -602 newcontent.append((1 / 12) * (-self.content[t + 2] + 16 * self.content[t + 1] - 30 * self.content[t] + 16 * self.content[t - 1] - self.content[t - 2])) -603 if (all([x is None for x in newcontent])): -604 raise Exception("Derivative is undefined at all timeslices") -605 return Corr(newcontent, padding=[2, 2]) -606 elif variant == 'log': -607 newcontent = [] -608 for t in range(self.T): -609 if (self.content[t] is None) or (self.content[t] <= 0): -610 newcontent.append(None) -611 else: -612 newcontent.append(np.log(self.content[t])) -613 if (all([x is None for x in newcontent])): -614 raise Exception("Log is undefined at all timeslices") -615 logcorr = Corr(newcontent) -616 return self * (logcorr.second_deriv('symmetric') + (logcorr.deriv('symmetric'))**2) -617 else: -618 raise Exception("Unknown variant.") +@@ -3907,89 +3943,89 @@ Available choice: symmetric, improved, log, default: symmetric577 def second_deriv(self, variant="symmetric"): +578 """Return the second derivative of the correlator with respect to x0. +579 +580 Parameters +581 ---------- +582 variant : str +583 decides which definition of the finite differences derivative is used. +584 Available choice: symmetric, improved, log, default: symmetric +585 """ +586 if self.N != 1: +587 raise Exception("second_deriv only implemented for one-dimensional correlators.") +588 if variant == "symmetric": +589 newcontent = [] +590 for t in range(1, self.T - 1): +591 if (self.content[t - 1] is None) or (self.content[t + 1] is None): +592 newcontent.append(None) +593 else: +594 newcontent.append((self.content[t + 1] - 2 * self.content[t] + self.content[t - 1])) +595 if (all([x is None for x in newcontent])): +596 raise Exception("Derivative is undefined at all timeslices") +597 return Corr(newcontent, padding=[1, 1]) +598 elif variant == "improved": +599 newcontent = [] +600 for t in range(2, self.T - 2): +601 if (self.content[t - 2] is None) or (self.content[t - 1] is None) or (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t + 2] is None): +602 newcontent.append(None) +603 else: +604 newcontent.append((1 / 12) * (-self.content[t + 2] + 16 * self.content[t + 1] - 30 * self.content[t] + 16 * self.content[t - 1] - self.content[t - 2])) +605 if (all([x is None for x in newcontent])): +606 raise Exception("Derivative is undefined at all timeslices") +607 return Corr(newcontent, padding=[2, 2]) +608 elif variant == 'log': +609 newcontent = [] +610 for t in range(self.T): +611 if (self.content[t] is None) or (self.content[t] <= 0): +612 newcontent.append(None) +613 else: +614 newcontent.append(np.log(self.content[t])) +615 if (all([x is None for x in newcontent])): +616 raise Exception("Log is undefined at all timeslices") +617 logcorr = Corr(newcontent) +618 return self * (logcorr.second_deriv('symmetric') + (logcorr.deriv('symmetric'))**2) +619 else: +620 raise Exception("Unknown variant.")
620 def m_eff(self, variant='log', guess=1.0): -621 """Returns the effective mass of the correlator as correlator object -622 -623 Parameters -624 ---------- -625 variant : str -626 log : uses the standard effective mass log(C(t) / C(t+1)) -627 cosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m. -628 sinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m. -629 See, e.g., arXiv:1205.5380 -630 arccosh : Uses the explicit form of the symmetrized correlator (not recommended) -631 logsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2 -632 guess : float -633 guess for the root finder, only relevant for the root variant -634 """ -635 if self.N != 1: -636 raise Exception('Correlator must be projected before getting m_eff') -637 if variant == 'log': -638 newcontent = [] -639 for t in range(self.T - 1): -640 if ((self.content[t] is None) or (self.content[t + 1] is None)) or (self.content[t + 1][0].value == 0): -641 newcontent.append(None) -642 elif self.content[t][0].value / self.content[t + 1][0].value < 0: +@@ -4023,39 +4059,39 @@ guess for the root finder, only relevant for the root variant622 def m_eff(self, variant='log', guess=1.0): +623 """Returns the effective mass of the correlator as correlator object +624 +625 Parameters +626 ---------- +627 variant : str +628 log : uses the standard effective mass log(C(t) / C(t+1)) +629 cosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m. +630 sinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m. +631 See, e.g., arXiv:1205.5380 +632 arccosh : Uses the explicit form of the symmetrized correlator (not recommended) +633 logsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2 +634 guess : float +635 guess for the root finder, only relevant for the root variant +636 """ +637 if self.N != 1: +638 raise Exception('Correlator must be projected before getting m_eff') +639 if variant == 'log': +640 newcontent = [] +641 for t in range(self.T - 1): +642 if ((self.content[t] is None) or (self.content[t + 1] is None)) or (self.content[t + 1][0].value == 0): 643 newcontent.append(None) -644 else: -645 newcontent.append(self.content[t] / self.content[t + 1]) -646 if (all([x is None for x in newcontent])): -647 raise Exception('m_eff is undefined at all timeslices') -648 -649 return np.log(Corr(newcontent, padding=[0, 1])) +644 elif self.content[t][0].value / self.content[t + 1][0].value < 0: +645 newcontent.append(None) +646 else: +647 newcontent.append(self.content[t] / self.content[t + 1]) +648 if (all([x is None for x in newcontent])): +649 raise Exception('m_eff is undefined at all timeslices') 650 -651 elif variant == 'logsym': -652 newcontent = [] -653 for t in range(1, self.T - 1): -654 if ((self.content[t - 1] is None) or (self.content[t + 1] is None)) or (self.content[t + 1][0].value == 0): -655 newcontent.append(None) -656 elif self.content[t - 1][0].value / self.content[t + 1][0].value < 0: +651 return np.log(Corr(newcontent, padding=[0, 1])) +652 +653 elif variant == 'logsym': +654 newcontent = [] +655 for t in range(1, self.T - 1): +656 if ((self.content[t - 1] is None) or (self.content[t + 1] is None)) or (self.content[t + 1][0].value == 0): 657 newcontent.append(None) -658 else: -659 newcontent.append(self.content[t - 1] / self.content[t + 1]) -660 if (all([x is None for x in newcontent])): -661 raise Exception('m_eff is undefined at all timeslices') -662 -663 return np.log(Corr(newcontent, padding=[1, 1])) / 2 +658 elif self.content[t - 1][0].value / self.content[t + 1][0].value < 0: +659 newcontent.append(None) +660 else: +661 newcontent.append(self.content[t - 1] / self.content[t + 1]) +662 if (all([x is None for x in newcontent])): +663 raise Exception('m_eff is undefined at all timeslices') 664 -665 elif variant in ['periodic', 'cosh', 'sinh']: -666 if variant in ['periodic', 'cosh']: -667 func = anp.cosh -668 else: -669 func = anp.sinh -670 -671 def root_function(x, d): -672 return func(x * (t - self.T / 2)) / func(x * (t + 1 - self.T / 2)) - d -673 -674 newcontent = [] -675 for t in range(self.T - 1): -676 if (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t + 1][0].value == 0): -677 newcontent.append(None) -678 # Fill the two timeslices in the middle of the lattice with their predecessors -679 elif variant == 'sinh' and t in [self.T / 2, self.T / 2 - 1]: -680 newcontent.append(newcontent[-1]) -681 elif self.content[t][0].value / self.content[t + 1][0].value < 0: -682 newcontent.append(None) -683 else: -684 newcontent.append(np.abs(find_root(self.content[t][0] / self.content[t + 1][0], root_function, guess=guess))) -685 if (all([x is None for x in newcontent])): -686 raise Exception('m_eff is undefined at all timeslices') -687 -688 return Corr(newcontent, padding=[0, 1]) +665 return np.log(Corr(newcontent, padding=[1, 1])) / 2 +666 +667 elif variant in ['periodic', 'cosh', 'sinh']: +668 if variant in ['periodic', 'cosh']: +669 func = anp.cosh +670 else: +671 func = anp.sinh +672 +673 def root_function(x, d): +674 return func(x * (t - self.T / 2)) / func(x * (t + 1 - self.T / 2)) - d +675 +676 newcontent = [] +677 for t in range(self.T - 1): +678 if (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t + 1][0].value == 0): +679 newcontent.append(None) +680 # Fill the two timeslices in the middle of the lattice with their predecessors +681 elif variant == 'sinh' and t in [self.T / 2, self.T / 2 - 1]: +682 newcontent.append(newcontent[-1]) +683 elif self.content[t][0].value / self.content[t + 1][0].value < 0: +684 newcontent.append(None) +685 else: +686 newcontent.append(np.abs(find_root(self.content[t][0] / self.content[t + 1][0], root_function, guess=guess))) +687 if (all([x is None for x in newcontent])): +688 raise Exception('m_eff is undefined at all timeslices') 689 -690 elif variant == 'arccosh': -691 newcontent = [] -692 for t in range(1, self.T - 1): -693 if (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t - 1] is None) or (self.content[t][0].value == 0): -694 newcontent.append(None) -695 else: -696 newcontent.append((self.content[t + 1] + self.content[t - 1]) / (2 * self.content[t])) -697 if (all([x is None for x in newcontent])): -698 raise Exception("m_eff is undefined at all timeslices") -699 return np.arccosh(Corr(newcontent, padding=[1, 1])) -700 -701 else: -702 raise Exception('Unknown variant.') +690 return Corr(newcontent, padding=[0, 1]) +691 +692 elif variant == 'arccosh': +693 newcontent = [] +694 for t in range(1, self.T - 1): +695 if (self.content[t] is None) or (self.content[t + 1] is None) or (self.content[t - 1] is None) or (self.content[t][0].value == 0): +696 newcontent.append(None) +697 else: +698 newcontent.append((self.content[t + 1] + self.content[t - 1]) / (2 * self.content[t])) +699 if (all([x is None for x in newcontent])): +700 raise Exception("m_eff is undefined at all timeslices") +701 return np.arccosh(Corr(newcontent, padding=[1, 1])) +702 +703 else: +704 raise Exception('Unknown variant.')
704 def fit(self, function, fitrange=None, silent=False, **kwargs): -705 r'''Fits function to the data -706 -707 Parameters -708 ---------- -709 function : obj -710 function to fit to the data. See fits.least_squares for details. -711 fitrange : list -712 Two element list containing the timeslices on which the fit is supposed to start and stop. -713 Caution: This range is inclusive as opposed to standard python indexing. -714 `fitrange=[4, 6]` corresponds to the three entries 4, 5 and 6. -715 If not specified, self.prange or all timeslices are used. -716 silent : bool -717 Decides whether output is printed to the standard output. -718 ''' -719 if self.N != 1: -720 raise Exception("Correlator must be projected before fitting") -721 -722 if fitrange is None: -723 if self.prange: -724 fitrange = self.prange -725 else: -726 fitrange = [0, self.T - 1] -727 else: -728 if not isinstance(fitrange, list): -729 raise Exception("fitrange has to be a list with two elements") -730 if len(fitrange) != 2: -731 raise Exception("fitrange has to have exactly two elements [fit_start, fit_stop]") -732 -733 xs = [x for x in range(fitrange[0], fitrange[1] + 1) if not self.content[x] is None] -734 ys = [self.content[x][0] for x in range(fitrange[0], fitrange[1] + 1) if not self.content[x] is None] -735 result = least_squares(xs, ys, function, silent=silent, **kwargs) -736 return result +@@ -4089,42 +4125,42 @@ Decides whether output is printed to the standard output.706 def fit(self, function, fitrange=None, silent=False, **kwargs): +707 r'''Fits function to the data +708 +709 Parameters +710 ---------- +711 function : obj +712 function to fit to the data. See fits.least_squares for details. +713 fitrange : list +714 Two element list containing the timeslices on which the fit is supposed to start and stop. +715 Caution: This range is inclusive as opposed to standard python indexing. +716 `fitrange=[4, 6]` corresponds to the three entries 4, 5 and 6. +717 If not specified, self.prange or all timeslices are used. +718 silent : bool +719 Decides whether output is printed to the standard output. +720 ''' +721 if self.N != 1: +722 raise Exception("Correlator must be projected before fitting") +723 +724 if fitrange is None: +725 if self.prange: +726 fitrange = self.prange +727 else: +728 fitrange = [0, self.T - 1] +729 else: +730 if not isinstance(fitrange, list): +731 raise Exception("fitrange has to be a list with two elements") +732 if len(fitrange) != 2: +733 raise Exception("fitrange has to have exactly two elements [fit_start, fit_stop]") +734 +735 xs = [x for x in range(fitrange[0], fitrange[1] + 1) if not self.content[x] is None] +736 ys = [self.content[x][0] for x in range(fitrange[0], fitrange[1] + 1) if not self.content[x] is None] +737 result = least_squares(xs, ys, function, silent=silent, **kwargs) +738 return result
738 def plateau(self, plateau_range=None, method="fit", auto_gamma=False): -739 """ Extract a plateau value from a Corr object -740 -741 Parameters -742 ---------- -743 plateau_range : list -744 list with two entries, indicating the first and the last timeslice -745 of the plateau region. -746 method : str -747 method to extract the plateau. -748 'fit' fits a constant to the plateau region -749 'avg', 'average' or 'mean' just average over the given timeslices. -750 auto_gamma : bool -751 apply gamma_method with default parameters to the Corr. Defaults to None -752 """ -753 if not plateau_range: -754 if self.prange: -755 plateau_range = self.prange -756 else: -757 raise Exception("no plateau range provided") -758 if self.N != 1: -759 raise Exception("Correlator must be projected before getting a plateau.") -760 if (all([self.content[t] is None for t in range(plateau_range[0], plateau_range[1] + 1)])): -761 raise Exception("plateau is undefined at all timeslices in plateaurange.") -762 if auto_gamma: -763 self.gamma_method() -764 if method == "fit": -765 def const_func(a, t): -766 return a[0] -767 return self.fit(const_func, plateau_range)[0] -768 elif method in ["avg", "average", "mean"]: -769 returnvalue = np.mean([item[0] for item in self.content[plateau_range[0]:plateau_range[1] + 1] if item is not None]) -770 return returnvalue -771 -772 else: -773 raise Exception("Unsupported plateau method: " + method) +@@ -4158,17 +4194,17 @@ apply gamma_method with default parameters to the Corr. Defaults to None740 def plateau(self, plateau_range=None, method="fit", auto_gamma=False): +741 """ Extract a plateau value from a Corr object +742 +743 Parameters +744 ---------- +745 plateau_range : list +746 list with two entries, indicating the first and the last timeslice +747 of the plateau region. +748 method : str +749 method to extract the plateau. +750 'fit' fits a constant to the plateau region +751 'avg', 'average' or 'mean' just average over the given timeslices. +752 auto_gamma : bool +753 apply gamma_method with default parameters to the Corr. Defaults to None +754 """ +755 if not plateau_range: +756 if self.prange: +757 plateau_range = self.prange +758 else: +759 raise Exception("no plateau range provided") +760 if self.N != 1: +761 raise Exception("Correlator must be projected before getting a plateau.") +762 if (all([self.content[t] is None for t in range(plateau_range[0], plateau_range[1] + 1)])): +763 raise Exception("plateau is undefined at all timeslices in plateaurange.") +764 if auto_gamma: +765 self.gamma_method() +766 if method == "fit": +767 def const_func(a, t): +768 return a[0] +769 return self.fit(const_func, plateau_range)[0] +770 elif method in ["avg", "average", "mean"]: +771 returnvalue = np.mean([item[0] for item in self.content[plateau_range[0]:plateau_range[1] + 1] if item is not None]) +772 return returnvalue +773 +774 else: +775 raise Exception("Unsupported plateau method: " + method)
775 def set_prange(self, prange): -776 """Sets the attribute prange of the Corr object.""" -777 if not len(prange) == 2: -778 raise Exception("prange must be a list or array with two values") -779 if not ((isinstance(prange[0], int)) and (isinstance(prange[1], int))): -780 raise Exception("Start and end point must be integers") -781 if not (0 <= prange[0] <= self.T and 0 <= prange[1] <= self.T and prange[0] < prange[1]): -782 raise Exception("Start and end point must define a range in the interval 0,T") -783 -784 self.prange = prange -785 return +@@ -4188,124 +4224,124 @@ apply gamma_method with default parameters to the Corr. Defaults to None777 def set_prange(self, prange): +778 """Sets the attribute prange of the Corr object.""" +779 if not len(prange) == 2: +780 raise Exception("prange must be a list or array with two values") +781 if not ((isinstance(prange[0], int)) and (isinstance(prange[1], int))): +782 raise Exception("Start and end point must be integers") +783 if not (0 <= prange[0] <= self.T and 0 <= prange[1] <= self.T and prange[0] < prange[1]): +784 raise Exception("Start and end point must define a range in the interval 0,T") +785 +786 self.prange = prange +787 return
787 def show(self, x_range=None, comp=None, y_range=None, logscale=False, plateau=None, fit_res=None, ylabel=None, save=None, auto_gamma=False, hide_sigma=None, references=None, title=None): -788 """Plots the correlator using the tag of the correlator as label if available. -789 -790 Parameters -791 ---------- -792 x_range : list -793 list of two values, determining the range of the x-axis e.g. [4, 8]. -794 comp : Corr or list of Corr -795 Correlator or list of correlators which are plotted for comparison. -796 The tags of these correlators are used as labels if available. -797 logscale : bool -798 Sets y-axis to logscale. -799 plateau : Obs -800 Plateau value to be visualized in the figure. -801 fit_res : Fit_result -802 Fit_result object to be visualized. -803 ylabel : str -804 Label for the y-axis. -805 save : str -806 path to file in which the figure should be saved. -807 auto_gamma : bool -808 Apply the gamma method with standard parameters to all correlators and plateau values before plotting. -809 hide_sigma : float -810 Hides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors. -811 references : list -812 List of floating point values that are displayed as horizontal lines for reference. -813 title : string -814 Optional title of the figure. -815 """ -816 if self.N != 1: -817 raise Exception("Correlator must be projected before plotting") -818 -819 if auto_gamma: -820 self.gamma_method() -821 -822 if x_range is None: -823 x_range = [0, self.T - 1] -824 -825 fig = plt.figure() -826 ax1 = fig.add_subplot(111) -827 -828 x, y, y_err = self.plottable() -829 if hide_sigma: -830 hide_from = np.argmax((hide_sigma * np.array(y_err[1:])) > np.abs(y[1:])) - 1 -831 else: -832 hide_from = None -833 ax1.errorbar(x[:hide_from], y[:hide_from], y_err[:hide_from], label=self.tag) -834 if logscale: -835 ax1.set_yscale('log') -836 else: -837 if y_range is None: -838 try: -839 y_min = min([(x[0].value - x[0].dvalue) for x in self.content[x_range[0]: x_range[1] + 1] if (x is not None) and x[0].dvalue < 2 * np.abs(x[0].value)]) -840 y_max = max([(x[0].value + x[0].dvalue) for x in self.content[x_range[0]: x_range[1] + 1] if (x is not None) and x[0].dvalue < 2 * np.abs(x[0].value)]) -841 ax1.set_ylim([y_min - 0.1 * (y_max - y_min), y_max + 0.1 * (y_max - y_min)]) -842 except Exception: -843 pass -844 else: -845 ax1.set_ylim(y_range) -846 if comp: -847 if isinstance(comp, (Corr, list)): -848 for corr in comp if isinstance(comp, list) else [comp]: -849 if auto_gamma: -850 corr.gamma_method() -851 x, y, y_err = corr.plottable() -852 if hide_sigma: -853 hide_from = np.argmax((hide_sigma * np.array(y_err[1:])) > np.abs(y[1:])) - 1 -854 else: -855 hide_from = None -856 ax1.errorbar(x[:hide_from], y[:hide_from], y_err[:hide_from], label=corr.tag, mfc=plt.rcParams['axes.facecolor']) -857 else: -858 raise Exception("'comp' must be a correlator or a list of correlators.") -859 -860 if plateau: -861 if isinstance(plateau, Obs): -862 if auto_gamma: -863 plateau.gamma_method() -864 ax1.axhline(y=plateau.value, linewidth=2, color=plt.rcParams['text.color'], alpha=0.6, marker=',', ls='--', label=str(plateau)) -865 ax1.axhspan(plateau.value - plateau.dvalue, plateau.value + plateau.dvalue, alpha=0.25, color=plt.rcParams['text.color'], ls='-') -866 else: -867 raise Exception("'plateau' must be an Obs") -868 -869 if references: -870 if isinstance(references, list): -871 for ref in references: -872 ax1.axhline(y=ref, linewidth=1, color=plt.rcParams['text.color'], alpha=0.6, marker=',', ls='--') -873 else: -874 raise Exception("'references' must be a list of floating pint values.") -875 -876 if self.prange: -877 ax1.axvline(self.prange[0], 0, 1, ls='-', marker=',') -878 ax1.axvline(self.prange[1], 0, 1, ls='-', marker=',') -879 -880 if fit_res: -881 x_samples = np.arange(x_range[0], x_range[1] + 1, 0.05) -882 ax1.plot(x_samples, -883 fit_res.fit_function([o.value for o in fit_res.fit_parameters], x_samples), -884 ls='-', marker=',', lw=2) -885 -886 ax1.set_xlabel(r'$x_0 / a$') -887 if ylabel: -888 ax1.set_ylabel(ylabel) -889 ax1.set_xlim([x_range[0] - 0.5, x_range[1] + 0.5]) -890 -891 handles, labels = ax1.get_legend_handles_labels() -892 if labels: -893 ax1.legend() -894 -895 if title: -896 plt.title(title) -897 -898 plt.draw() +@@ -4353,34 +4389,34 @@ Optional title of the figure.789 def show(self, x_range=None, comp=None, y_range=None, logscale=False, plateau=None, fit_res=None, ylabel=None, save=None, auto_gamma=False, hide_sigma=None, references=None, title=None): +790 """Plots the correlator using the tag of the correlator as label if available. +791 +792 Parameters +793 ---------- +794 x_range : list +795 list of two values, determining the range of the x-axis e.g. [4, 8]. +796 comp : Corr or list of Corr +797 Correlator or list of correlators which are plotted for comparison. +798 The tags of these correlators are used as labels if available. +799 logscale : bool +800 Sets y-axis to logscale. +801 plateau : Obs +802 Plateau value to be visualized in the figure. +803 fit_res : Fit_result +804 Fit_result object to be visualized. +805 ylabel : str +806 Label for the y-axis. +807 save : str +808 path to file in which the figure should be saved. +809 auto_gamma : bool +810 Apply the gamma method with standard parameters to all correlators and plateau values before plotting. +811 hide_sigma : float +812 Hides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors. +813 references : list +814 List of floating point values that are displayed as horizontal lines for reference. +815 title : string +816 Optional title of the figure. +817 """ +818 if self.N != 1: +819 raise Exception("Correlator must be projected before plotting") +820 +821 if auto_gamma: +822 self.gamma_method() +823 +824 if x_range is None: +825 x_range = [0, self.T - 1] +826 +827 fig = plt.figure() +828 ax1 = fig.add_subplot(111) +829 +830 x, y, y_err = self.plottable() +831 if hide_sigma: +832 hide_from = np.argmax((hide_sigma * np.array(y_err[1:])) > np.abs(y[1:])) - 1 +833 else: +834 hide_from = None +835 ax1.errorbar(x[:hide_from], y[:hide_from], y_err[:hide_from], label=self.tag) +836 if logscale: +837 ax1.set_yscale('log') +838 else: +839 if y_range is None: +840 try: +841 y_min = min([(x[0].value - x[0].dvalue) for x in self.content[x_range[0]: x_range[1] + 1] if (x is not None) and x[0].dvalue < 2 * np.abs(x[0].value)]) +842 y_max = max([(x[0].value + x[0].dvalue) for x in self.content[x_range[0]: x_range[1] + 1] if (x is not None) and x[0].dvalue < 2 * np.abs(x[0].value)]) +843 ax1.set_ylim([y_min - 0.1 * (y_max - y_min), y_max + 0.1 * (y_max - y_min)]) +844 except Exception: +845 pass +846 else: +847 ax1.set_ylim(y_range) +848 if comp: +849 if isinstance(comp, (Corr, list)): +850 for corr in comp if isinstance(comp, list) else [comp]: +851 if auto_gamma: +852 corr.gamma_method() +853 x, y, y_err = corr.plottable() +854 if hide_sigma: +855 hide_from = np.argmax((hide_sigma * np.array(y_err[1:])) > np.abs(y[1:])) - 1 +856 else: +857 hide_from = None +858 ax1.errorbar(x[:hide_from], y[:hide_from], y_err[:hide_from], label=corr.tag, mfc=plt.rcParams['axes.facecolor']) +859 else: +860 raise Exception("'comp' must be a correlator or a list of correlators.") +861 +862 if plateau: +863 if isinstance(plateau, Obs): +864 if auto_gamma: +865 plateau.gamma_method() +866 ax1.axhline(y=plateau.value, linewidth=2, color=plt.rcParams['text.color'], alpha=0.6, marker=',', ls='--', label=str(plateau)) +867 ax1.axhspan(plateau.value - plateau.dvalue, plateau.value + plateau.dvalue, alpha=0.25, color=plt.rcParams['text.color'], ls='-') +868 else: +869 raise Exception("'plateau' must be an Obs") +870 +871 if references: +872 if isinstance(references, list): +873 for ref in references: +874 ax1.axhline(y=ref, linewidth=1, color=plt.rcParams['text.color'], alpha=0.6, marker=',', ls='--') +875 else: +876 raise Exception("'references' must be a list of floating pint values.") +877 +878 if self.prange: +879 ax1.axvline(self.prange[0], 0, 1, ls='-', marker=',') +880 ax1.axvline(self.prange[1], 0, 1, ls='-', marker=',') +881 +882 if fit_res: +883 x_samples = np.arange(x_range[0], x_range[1] + 1, 0.05) +884 ax1.plot(x_samples, +885 fit_res.fit_function([o.value for o in fit_res.fit_parameters], x_samples), +886 ls='-', marker=',', lw=2) +887 +888 ax1.set_xlabel(r'$x_0 / a$') +889 if ylabel: +890 ax1.set_ylabel(ylabel) +891 ax1.set_xlim([x_range[0] - 0.5, x_range[1] + 0.5]) +892 +893 handles, labels = ax1.get_legend_handles_labels() +894 if labels: +895 ax1.legend() +896 +897 if title: +898 plt.title(title) 899 -900 if save: -901 if isinstance(save, str): -902 fig.savefig(save, bbox_inches='tight') -903 else: -904 raise Exception("'save' has to be a string.") +900 plt.draw() +901 +902 if save: +903 if isinstance(save, str): +904 fig.savefig(save, bbox_inches='tight') +905 else: +906 raise Exception("'save' has to be a string.")
906 def spaghetti_plot(self, logscale=True): -907 """Produces a spaghetti plot of the correlator suited to monitor exceptional configurations. -908 -909 Parameters -910 ---------- -911 logscale : bool -912 Determines whether the scale of the y-axis is logarithmic or standard. -913 """ -914 if self.N != 1: -915 raise Exception("Correlator needs to be projected first.") -916 -917 mc_names = list(set([item for sublist in [sum(map(o[0].e_content.get, o[0].mc_names), []) for o in self.content if o is not None] for item in sublist])) -918 x0_vals = [n for (n, o) in zip(np.arange(self.T), self.content) if o is not None] -919 -920 for name in mc_names: -921 data = np.array([o[0].deltas[name] + o[0].r_values[name] for o in self.content if o is not None]).T -922 -923 fig = plt.figure() -924 ax = fig.add_subplot(111) -925 for dat in data: -926 ax.plot(x0_vals, dat, ls='-', marker='') -927 -928 if logscale is True: -929 ax.set_yscale('log') -930 -931 ax.set_xlabel(r'$x_0 / a$') -932 plt.title(name) -933 plt.draw() +@@ -4407,29 +4443,29 @@ Determines whether the scale of the y-axis is logarithmic or standard.908 def spaghetti_plot(self, logscale=True): +909 """Produces a spaghetti plot of the correlator suited to monitor exceptional configurations. +910 +911 Parameters +912 ---------- +913 logscale : bool +914 Determines whether the scale of the y-axis is logarithmic or standard. +915 """ +916 if self.N != 1: +917 raise Exception("Correlator needs to be projected first.") +918 +919 mc_names = list(set([item for sublist in [sum(map(o[0].e_content.get, o[0].mc_names), []) for o in self.content if o is not None] for item in sublist])) +920 x0_vals = [n for (n, o) in zip(np.arange(self.T), self.content) if o is not None] +921 +922 for name in mc_names: +923 data = np.array([o[0].deltas[name] + o[0].r_values[name] for o in self.content if o is not None]).T +924 +925 fig = plt.figure() +926 ax = fig.add_subplot(111) +927 for dat in data: +928 ax.plot(x0_vals, dat, ls='-', marker='') +929 +930 if logscale is True: +931 ax.set_yscale('log') +932 +933 ax.set_xlabel(r'$x_0 / a$') +934 plt.title(name) +935 plt.draw()
935 def dump(self, filename, datatype="json.gz", **kwargs): -936 """Dumps the Corr into a file of chosen type -937 Parameters -938 ---------- -939 filename : str -940 Name of the file to be saved. -941 datatype : str -942 Format of the exported file. Supported formats include -943 "json.gz" and "pickle" -944 path : str -945 specifies a custom path for the file (default '.') -946 """ -947 if datatype == "json.gz": -948 from .input.json import dump_to_json -949 if 'path' in kwargs: -950 file_name = kwargs.get('path') + '/' + filename -951 else: -952 file_name = filename -953 dump_to_json(self, file_name) -954 elif datatype == "pickle": -955 dump_object(self, filename, **kwargs) -956 else: -957 raise Exception("Unknown datatype " + str(datatype)) +@@ -4461,8 +4497,8 @@ specifies a custom path for the file (default '.')937 def dump(self, filename, datatype="json.gz", **kwargs): +938 """Dumps the Corr into a file of chosen type +939 Parameters +940 ---------- +941 filename : str +942 Name of the file to be saved. +943 datatype : str +944 Format of the exported file. Supported formats include +945 "json.gz" and "pickle" +946 path : str +947 specifies a custom path for the file (default '.') +948 """ +949 if datatype == "json.gz": +950 from .input.json import dump_to_json +951 if 'path' in kwargs: +952 file_name = kwargs.get('path') + '/' + filename +953 else: +954 file_name = filename +955 dump_to_json(self, file_name) +956 elif datatype == "pickle": +957 dump_object(self, filename, **kwargs) +958 else: +959 raise Exception("Unknown datatype " + str(datatype))
959 def print(self, print_range=None): -960 print(self.__repr__(print_range)) + @@ -4480,8 +4516,8 @@ specifies a custom path for the file (default '.')
1126 def sqrt(self): -1127 return self ** 0.5 + @@ -4499,9 +4535,9 @@ specifies a custom path for the file (default '.')
1129 def log(self): -1130 newcontent = [None if _check_for_none(self, item) else np.log(item) for item in self.content] -1131 return Corr(newcontent, prange=self.prange) + @@ -4519,9 +4555,9 @@ specifies a custom path for the file (default '.')
1133 def exp(self): -1134 newcontent = [None if _check_for_none(self, item) else np.exp(item) for item in self.content] -1135 return Corr(newcontent, prange=self.prange) + @@ -4539,8 +4575,8 @@ specifies a custom path for the file (default '.')
1150 def sin(self): -1151 return self._apply_func_to_corr(np.sin) + @@ -4558,8 +4594,8 @@ specifies a custom path for the file (default '.')
1153 def cos(self): -1154 return self._apply_func_to_corr(np.cos) + @@ -4577,8 +4613,8 @@ specifies a custom path for the file (default '.')
1156 def tan(self): -1157 return self._apply_func_to_corr(np.tan) + @@ -4596,8 +4632,8 @@ specifies a custom path for the file (default '.')
1159 def sinh(self): -1160 return self._apply_func_to_corr(np.sinh) + @@ -4615,8 +4651,8 @@ specifies a custom path for the file (default '.')
1162 def cosh(self): -1163 return self._apply_func_to_corr(np.cosh) + @@ -4634,8 +4670,8 @@ specifies a custom path for the file (default '.')
1165 def tanh(self): -1166 return self._apply_func_to_corr(np.tanh) + @@ -4653,8 +4689,8 @@ specifies a custom path for the file (default '.')
1168 def arcsin(self): -1169 return self._apply_func_to_corr(np.arcsin) + @@ -4672,8 +4708,8 @@ specifies a custom path for the file (default '.')
1171 def arccos(self): -1172 return self._apply_func_to_corr(np.arccos) + @@ -4691,8 +4727,8 @@ specifies a custom path for the file (default '.')
1174 def arctan(self): -1175 return self._apply_func_to_corr(np.arctan) + @@ -4710,8 +4746,8 @@ specifies a custom path for the file (default '.')
1177 def arcsinh(self): -1178 return self._apply_func_to_corr(np.arcsinh) + @@ -4729,8 +4765,8 @@ specifies a custom path for the file (default '.')
1180 def arccosh(self): -1181 return self._apply_func_to_corr(np.arccosh) + @@ -4748,8 +4784,8 @@ specifies a custom path for the file (default '.')
1183 def arctanh(self): -1184 return self._apply_func_to_corr(np.arctanh) + @@ -4767,62 +4803,62 @@ specifies a custom path for the file (default '.')
1219 def prune(self, Ntrunc, tproj=3, t0proj=2, basematrix=None): -1220 r''' Project large correlation matrix to lowest states -1221 -1222 This method can be used to reduce the size of an (N x N) correlation matrix -1223 to (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise -1224 is still small. -1225 -1226 Parameters -1227 ---------- -1228 Ntrunc: int -1229 Rank of the target matrix. -1230 tproj: int -1231 Time where the eigenvectors are evaluated, corresponds to ts in the GEVP method. -1232 The default value is 3. -1233 t0proj: int -1234 Time where the correlation matrix is inverted. Choosing t0proj=1 is strongly -1235 discouraged for O(a) improved theories, since the correctness of the procedure -1236 cannot be granted in this case. The default value is 2. -1237 basematrix : Corr -1238 Correlation matrix that is used to determine the eigenvectors of the -1239 lowest states based on a GEVP. basematrix is taken to be the Corr itself if -1240 is is not specified. -1241 -1242 Notes -1243 ----- -1244 We have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving -1245 the GEVP $$C(t) v_n(t, t_0) = \lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \equiv t_\mathrm{proj}$ -1246 and $t_0 \equiv t_{0, \mathrm{proj}}$. The target matrix is projected onto the subspace of the -1247 resulting eigenvectors $v_n, n=1,\dots,N_\mathrm{trunc}$ via -1248 $$G^\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large -1249 correlation matrix and to remove some noise that is added by irrelevant operators. -1250 This may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated -1251 bound $t_0 \leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$. -1252 ''' -1253 -1254 if self.N == 1: -1255 raise Exception('Method cannot be applied to one-dimensional correlators.') -1256 if basematrix is None: -1257 basematrix = self -1258 if Ntrunc >= basematrix.N: -1259 raise Exception('Cannot truncate using Ntrunc <= %d' % (basematrix.N)) -1260 if basematrix.N != self.N: -1261 raise Exception('basematrix and targetmatrix have to be of the same size.') -1262 -1263 evecs = basematrix.GEVP(t0proj, tproj, sort=None)[:Ntrunc] +diff --git a/docs/pyerrors/fits.html b/docs/pyerrors/fits.html index 15ed89b9..0be3cb04 100644 --- a/docs/pyerrors/fits.html +++ b/docs/pyerrors/fits.html @@ -61,6 +61,9 @@1221 def prune(self, Ntrunc, tproj=3, t0proj=2, basematrix=None): +1222 r''' Project large correlation matrix to lowest states +1223 +1224 This method can be used to reduce the size of an (N x N) correlation matrix +1225 to (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise +1226 is still small. +1227 +1228 Parameters +1229 ---------- +1230 Ntrunc: int +1231 Rank of the target matrix. +1232 tproj: int +1233 Time where the eigenvectors are evaluated, corresponds to ts in the GEVP method. +1234 The default value is 3. +1235 t0proj: int +1236 Time where the correlation matrix is inverted. Choosing t0proj=1 is strongly +1237 discouraged for O(a) improved theories, since the correctness of the procedure +1238 cannot be granted in this case. The default value is 2. +1239 basematrix : Corr +1240 Correlation matrix that is used to determine the eigenvectors of the +1241 lowest states based on a GEVP. basematrix is taken to be the Corr itself if +1242 is is not specified. +1243 +1244 Notes +1245 ----- +1246 We have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving +1247 the GEVP $$C(t) v_n(t, t_0) = \lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \equiv t_\mathrm{proj}$ +1248 and $t_0 \equiv t_{0, \mathrm{proj}}$. The target matrix is projected onto the subspace of the +1249 resulting eigenvectors $v_n, n=1,\dots,N_\mathrm{trunc}$ via +1250 $$G^\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large +1251 correlation matrix and to remove some noise that is added by irrelevant operators. +1252 This may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated +1253 bound $t_0 \leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$. +1254 ''' +1255 +1256 if self.N == 1: +1257 raise Exception('Method cannot be applied to one-dimensional correlators.') +1258 if basematrix is None: +1259 basematrix = self +1260 if Ntrunc >= basematrix.N: +1261 raise Exception('Cannot truncate using Ntrunc <= %d' % (basematrix.N)) +1262 if basematrix.N != self.N: +1263 raise Exception('basematrix and targetmatrix have to be of the same size.') 1264 -1265 tmpmat = np.empty((Ntrunc, Ntrunc), dtype=object) -1266 rmat = [] -1267 for t in range(basematrix.T): -1268 for i in range(Ntrunc): -1269 for j in range(Ntrunc): -1270 tmpmat[i][j] = evecs[i].T @ self[t] @ evecs[j] -1271 rmat.append(np.copy(tmpmat)) -1272 -1273 newcontent = [None if (self.content[t] is None) else rmat[t] for t in range(self.T)] -1274 return Corr(newcontent) +1265 evecs = basematrix.GEVP(t0proj, tproj, sort=None)[:Ntrunc] +1266 +1267 tmpmat = np.empty((Ntrunc, Ntrunc), dtype=object) +1268 rmat = [] +1269 for t in range(basematrix.T): +1270 for i in range(Ntrunc): +1271 for j in range(Ntrunc): +1272 tmpmat[i][j] = evecs[i].T @ self[t] @ evecs[j] +1273 rmat.append(np.copy(tmpmat)) +1274 +1275 newcontent = [None if (self.content[t] is None) else rmat[t] for t in range(self.T)] +1276 return Corr(newcontent)gamma_method ++ gm + @@ -154,754 +157,756 @@ 46 """Apply the gamma method to all fit parameters""" 47 [o.gamma_method(**kwargs) for o in self.fit_parameters] 48 - 49 def __str__(self): - 50 my_str = 'Goodness of fit:\n' - 51 if hasattr(self, 'chisquare_by_dof'): - 52 my_str += '\u03C7\u00b2/d.o.f. = ' + f'{self.chisquare_by_dof:2.6f}' + '\n' - 53 elif hasattr(self, 'residual_variance'): - 54 my_str += 'residual variance = ' + f'{self.residual_variance:2.6f}' + '\n' - 55 if hasattr(self, 'chisquare_by_expected_chisquare'): - 56 my_str += '\u03C7\u00b2/\u03C7\u00b2exp = ' + f'{self.chisquare_by_expected_chisquare:2.6f}' + '\n' - 57 if hasattr(self, 'p_value'): - 58 my_str += 'p-value = ' + f'{self.p_value:2.4f}' + '\n' - 59 if hasattr(self, 't2_p_value'): - 60 my_str += 't\u00B2p-value = ' + f'{self.t2_p_value:2.4f}' + '\n' - 61 my_str += 'Fit parameters:\n' - 62 for i_par, par in enumerate(self.fit_parameters): - 63 my_str += str(i_par) + '\t' + ' ' * int(par >= 0) + str(par).rjust(int(par < 0.0)) + '\n' - 64 return my_str - 65 - 66 def __repr__(self): - 67 m = max(map(len, list(self.__dict__.keys()))) + 1 - 68 return '\n'.join([key.rjust(m) + ': ' + repr(value) for key, value in sorted(self.__dict__.items())]) - 69 - 70 - 71def least_squares(x, y, func, priors=None, silent=False, **kwargs): - 72 r'''Performs a non-linear fit to y = func(x). - 73 - 74 Parameters - 75 ---------- - 76 x : list - 77 list of floats. - 78 y : list - 79 list of Obs. - 80 func : object - 81 fit function, has to be of the form - 82 - 83 ```python - 84 import autograd.numpy as anp - 85 - 86 def func(a, x): - 87 return a[0] + a[1] * x + a[2] * anp.sinh(x) - 88 ``` - 89 - 90 For multiple x values func can be of the form + 49 gm = gamma_method + 50 + 51 def __str__(self): + 52 my_str = 'Goodness of fit:\n' + 53 if hasattr(self, 'chisquare_by_dof'): + 54 my_str += '\u03C7\u00b2/d.o.f. = ' + f'{self.chisquare_by_dof:2.6f}' + '\n' + 55 elif hasattr(self, 'residual_variance'): + 56 my_str += 'residual variance = ' + f'{self.residual_variance:2.6f}' + '\n' + 57 if hasattr(self, 'chisquare_by_expected_chisquare'): + 58 my_str += '\u03C7\u00b2/\u03C7\u00b2exp = ' + f'{self.chisquare_by_expected_chisquare:2.6f}' + '\n' + 59 if hasattr(self, 'p_value'): + 60 my_str += 'p-value = ' + f'{self.p_value:2.4f}' + '\n' + 61 if hasattr(self, 't2_p_value'): + 62 my_str += 't\u00B2p-value = ' + f'{self.t2_p_value:2.4f}' + '\n' + 63 my_str += 'Fit parameters:\n' + 64 for i_par, par in enumerate(self.fit_parameters): + 65 my_str += str(i_par) + '\t' + ' ' * int(par >= 0) + str(par).rjust(int(par < 0.0)) + '\n' + 66 return my_str + 67 + 68 def __repr__(self): + 69 m = max(map(len, list(self.__dict__.keys()))) + 1 + 70 return '\n'.join([key.rjust(m) + ': ' + repr(value) for key, value in sorted(self.__dict__.items())]) + 71 + 72 + 73def least_squares(x, y, func, priors=None, silent=False, **kwargs): + 74 r'''Performs a non-linear fit to y = func(x). + 75 + 76 Parameters + 77 ---------- + 78 x : list + 79 list of floats. + 80 y : list + 81 list of Obs. + 82 func : object + 83 fit function, has to be of the form + 84 + 85 ```python + 86 import autograd.numpy as anp + 87 + 88 def func(a, x): + 89 return a[0] + a[1] * x + a[2] * anp.sinh(x) + 90 ``` 91 - 92 ```python - 93 def func(a, x): - 94 (x1, x2) = x - 95 return a[0] * x1 ** 2 + a[1] * x2 - 96 ``` - 97 - 98 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation - 99 will not work. -100 priors : list, optional -101 priors has to be a list with an entry for every parameter in the fit. The entries can either be -102 Obs (e.g. results from a previous fit) or strings containing a value and an error formatted like -103 0.548(23), 500(40) or 0.5(0.4) -104 silent : bool, optional -105 If true all output to the console is omitted (default False). -106 initial_guess : list -107 can provide an initial guess for the input parameters. Relevant for -108 non-linear fits with many parameters. In case of correlated fits the guess is used to perform -109 an uncorrelated fit which then serves as guess for the correlated fit. -110 method : str, optional -111 can be used to choose an alternative method for the minimization of chisquare. -112 The possible methods are the ones which can be used for scipy.optimize.minimize and -113 migrad of iminuit. If no method is specified, Levenberg-Marquard is used. -114 Reliable alternatives are migrad, Powell and Nelder-Mead. -115 correlated_fit : bool -116 If True, use the full inverse covariance matrix in the definition of the chisquare cost function. -117 For details about how the covariance matrix is estimated see `pyerrors.obs.covariance`. -118 In practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix). -119 This procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning). -120 At the moment this option only works for `prior==None` and when no `method` is given. -121 expected_chisquare : bool -122 If True estimates the expected chisquare which is -123 corrected by effects caused by correlated input data (default False). -124 resplot : bool -125 If True, a plot which displays fit, data and residuals is generated (default False). -126 qqplot : bool -127 If True, a quantile-quantile plot of the fit result is generated (default False). -128 num_grad : bool -129 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). -130 ''' -131 if priors is not None: -132 return _prior_fit(x, y, func, priors, silent=silent, **kwargs) -133 else: -134 return _standard_fit(x, y, func, silent=silent, **kwargs) -135 -136 -137def total_least_squares(x, y, func, silent=False, **kwargs): -138 r'''Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters. -139 -140 Parameters -141 ---------- -142 x : list -143 list of Obs, or a tuple of lists of Obs -144 y : list -145 list of Obs. The dvalues of the Obs are used as x- and yerror for the fit. -146 func : object -147 func has to be of the form -148 -149 ```python -150 import autograd.numpy as anp -151 -152 def func(a, x): -153 return a[0] + a[1] * x + a[2] * anp.sinh(x) -154 ``` -155 -156 For multiple x values func can be of the form + 92 For multiple x values func can be of the form + 93 + 94 ```python + 95 def func(a, x): + 96 (x1, x2) = x + 97 return a[0] * x1 ** 2 + a[1] * x2 + 98 ``` + 99 +100 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation +101 will not work. +102 priors : list, optional +103 priors has to be a list with an entry for every parameter in the fit. The entries can either be +104 Obs (e.g. results from a previous fit) or strings containing a value and an error formatted like +105 0.548(23), 500(40) or 0.5(0.4) +106 silent : bool, optional +107 If true all output to the console is omitted (default False). +108 initial_guess : list +109 can provide an initial guess for the input parameters. Relevant for +110 non-linear fits with many parameters. In case of correlated fits the guess is used to perform +111 an uncorrelated fit which then serves as guess for the correlated fit. +112 method : str, optional +113 can be used to choose an alternative method for the minimization of chisquare. +114 The possible methods are the ones which can be used for scipy.optimize.minimize and +115 migrad of iminuit. If no method is specified, Levenberg-Marquard is used. +116 Reliable alternatives are migrad, Powell and Nelder-Mead. +117 correlated_fit : bool +118 If True, use the full inverse covariance matrix in the definition of the chisquare cost function. +119 For details about how the covariance matrix is estimated see `pyerrors.obs.covariance`. +120 In practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix). +121 This procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning). +122 At the moment this option only works for `prior==None` and when no `method` is given. +123 expected_chisquare : bool +124 If True estimates the expected chisquare which is +125 corrected by effects caused by correlated input data (default False). +126 resplot : bool +127 If True, a plot which displays fit, data and residuals is generated (default False). +128 qqplot : bool +129 If True, a quantile-quantile plot of the fit result is generated (default False). +130 num_grad : bool +131 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). +132 ''' +133 if priors is not None: +134 return _prior_fit(x, y, func, priors, silent=silent, **kwargs) +135 else: +136 return _standard_fit(x, y, func, silent=silent, **kwargs) +137 +138 +139def total_least_squares(x, y, func, silent=False, **kwargs): +140 r'''Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters. +141 +142 Parameters +143 ---------- +144 x : list +145 list of Obs, or a tuple of lists of Obs +146 y : list +147 list of Obs. The dvalues of the Obs are used as x- and yerror for the fit. +148 func : object +149 func has to be of the form +150 +151 ```python +152 import autograd.numpy as anp +153 +154 def func(a, x): +155 return a[0] + a[1] * x + a[2] * anp.sinh(x) +156 ``` 157 -158 ```python -159 def func(a, x): -160 (x1, x2) = x -161 return a[0] * x1 ** 2 + a[1] * x2 -162 ``` -163 -164 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation -165 will not work. -166 silent : bool, optional -167 If true all output to the console is omitted (default False). -168 initial_guess : list -169 can provide an initial guess for the input parameters. Relevant for non-linear -170 fits with many parameters. -171 expected_chisquare : bool -172 If true prints the expected chisquare which is -173 corrected by effects caused by correlated input data. -174 This can take a while as the full correlation matrix -175 has to be calculated (default False). -176 num_grad : bool -177 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). -178 -179 Notes -180 ----- -181 Based on the orthogonal distance regression module of scipy -182 ''' -183 -184 output = Fit_result() +158 For multiple x values func can be of the form +159 +160 ```python +161 def func(a, x): +162 (x1, x2) = x +163 return a[0] * x1 ** 2 + a[1] * x2 +164 ``` +165 +166 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation +167 will not work. +168 silent : bool, optional +169 If true all output to the console is omitted (default False). +170 initial_guess : list +171 can provide an initial guess for the input parameters. Relevant for non-linear +172 fits with many parameters. +173 expected_chisquare : bool +174 If true prints the expected chisquare which is +175 corrected by effects caused by correlated input data. +176 This can take a while as the full correlation matrix +177 has to be calculated (default False). +178 num_grad : bool +179 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). +180 +181 Notes +182 ----- +183 Based on the orthogonal distance regression module of scipy +184 ''' 185 -186 output.fit_function = func +186 output = Fit_result() 187 -188 x = np.array(x) +188 output.fit_function = func 189 -190 x_shape = x.shape +190 x = np.array(x) 191 -192 if kwargs.get('num_grad') is True: -193 jacobian = num_jacobian -194 hessian = num_hessian -195 else: -196 jacobian = auto_jacobian -197 hessian = auto_hessian -198 -199 if not callable(func): -200 raise TypeError('func has to be a function.') -201 -202 for i in range(42): -203 try: -204 func(np.arange(i), x.T[0]) -205 except TypeError: -206 continue -207 except IndexError: +192 x_shape = x.shape +193 +194 if kwargs.get('num_grad') is True: +195 jacobian = num_jacobian +196 hessian = num_hessian +197 else: +198 jacobian = auto_jacobian +199 hessian = auto_hessian +200 +201 if not callable(func): +202 raise TypeError('func has to be a function.') +203 +204 for i in range(42): +205 try: +206 func(np.arange(i), x.T[0]) +207 except TypeError: 208 continue -209 else: -210 break -211 else: -212 raise RuntimeError("Fit function is not valid.") -213 -214 n_parms = i -215 if not silent: -216 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) -217 -218 x_f = np.vectorize(lambda o: o.value)(x) -219 dx_f = np.vectorize(lambda o: o.dvalue)(x) -220 y_f = np.array([o.value for o in y]) -221 dy_f = np.array([o.dvalue for o in y]) -222 -223 if np.any(np.asarray(dx_f) <= 0.0): -224 raise Exception('No x errors available, run the gamma method first.') -225 -226 if np.any(np.asarray(dy_f) <= 0.0): -227 raise Exception('No y errors available, run the gamma method first.') -228 -229 if 'initial_guess' in kwargs: -230 x0 = kwargs.get('initial_guess') -231 if len(x0) != n_parms: -232 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) -233 else: -234 x0 = [1] * n_parms -235 -236 data = RealData(x_f, y_f, sx=dx_f, sy=dy_f) -237 model = Model(func) -238 odr = ODR(data, model, x0, partol=np.finfo(np.float64).eps) -239 odr.set_job(fit_type=0, deriv=1) -240 out = odr.run() -241 -242 output.residual_variance = out.res_var +209 except IndexError: +210 continue +211 else: +212 break +213 else: +214 raise RuntimeError("Fit function is not valid.") +215 +216 n_parms = i +217 if not silent: +218 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) +219 +220 x_f = np.vectorize(lambda o: o.value)(x) +221 dx_f = np.vectorize(lambda o: o.dvalue)(x) +222 y_f = np.array([o.value for o in y]) +223 dy_f = np.array([o.dvalue for o in y]) +224 +225 if np.any(np.asarray(dx_f) <= 0.0): +226 raise Exception('No x errors available, run the gamma method first.') +227 +228 if np.any(np.asarray(dy_f) <= 0.0): +229 raise Exception('No y errors available, run the gamma method first.') +230 +231 if 'initial_guess' in kwargs: +232 x0 = kwargs.get('initial_guess') +233 if len(x0) != n_parms: +234 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) +235 else: +236 x0 = [1] * n_parms +237 +238 data = RealData(x_f, y_f, sx=dx_f, sy=dy_f) +239 model = Model(func) +240 odr = ODR(data, model, x0, partol=np.finfo(np.float64).eps) +241 odr.set_job(fit_type=0, deriv=1) +242 out = odr.run() 243 -244 output.method = 'ODR' +244 output.residual_variance = out.res_var 245 -246 output.message = out.stopreason +246 output.method = 'ODR' 247 -248 output.xplus = out.xplus +248 output.message = out.stopreason 249 -250 if not silent: -251 print('Method: ODR') -252 print(*out.stopreason) -253 print('Residual variance:', output.residual_variance) -254 -255 if out.info > 3: -256 raise Exception('The minimization procedure did not converge.') -257 -258 m = x_f.size +250 output.xplus = out.xplus +251 +252 if not silent: +253 print('Method: ODR') +254 print(*out.stopreason) +255 print('Residual variance:', output.residual_variance) +256 +257 if out.info > 3: +258 raise Exception('The minimization procedure did not converge.') 259 -260 def odr_chisquare(p): -261 model = func(p[:n_parms], p[n_parms:].reshape(x_shape)) -262 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((x_f - p[n_parms:].reshape(x_shape)) / dx_f) ** 2) -263 return chisq -264 -265 if kwargs.get('expected_chisquare') is True: -266 W = np.diag(1 / np.asarray(np.concatenate((dy_f.ravel(), dx_f.ravel())))) -267 -268 if kwargs.get('covariance') is not None: -269 cov = kwargs.get('covariance') -270 else: -271 cov = covariance(np.concatenate((y, x.ravel()))) -272 -273 number_of_x_parameters = int(m / x_f.shape[-1]) +260 m = x_f.size +261 +262 def odr_chisquare(p): +263 model = func(p[:n_parms], p[n_parms:].reshape(x_shape)) +264 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((x_f - p[n_parms:].reshape(x_shape)) / dx_f) ** 2) +265 return chisq +266 +267 if kwargs.get('expected_chisquare') is True: +268 W = np.diag(1 / np.asarray(np.concatenate((dy_f.ravel(), dx_f.ravel())))) +269 +270 if kwargs.get('covariance') is not None: +271 cov = kwargs.get('covariance') +272 else: +273 cov = covariance(np.concatenate((y, x.ravel()))) 274 -275 old_jac = jacobian(func)(out.beta, out.xplus) -276 fused_row1 = np.concatenate((old_jac, np.concatenate((number_of_x_parameters * [np.zeros(old_jac.shape)]), axis=0))) -277 fused_row2 = np.concatenate((jacobian(lambda x, y: func(y, x))(out.xplus, out.beta).reshape(x_f.shape[-1], x_f.shape[-1] * number_of_x_parameters), np.identity(number_of_x_parameters * old_jac.shape[0]))) -278 new_jac = np.concatenate((fused_row1, fused_row2), axis=1) -279 -280 A = W @ new_jac -281 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T -282 expected_chisquare = np.trace((np.identity(P_phi.shape[0]) - P_phi) @ W @ cov @ W) -283 if expected_chisquare <= 0.0: -284 warnings.warn("Negative expected_chisquare.", RuntimeWarning) -285 expected_chisquare = np.abs(expected_chisquare) -286 output.chisquare_by_expected_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) / expected_chisquare -287 if not silent: -288 print('chisquare/expected_chisquare:', -289 output.chisquare_by_expected_chisquare) -290 -291 fitp = out.beta -292 try: -293 hess = hessian(odr_chisquare)(np.concatenate((fitp, out.xplus.ravel()))) -294 except TypeError: -295 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None -296 -297 def odr_chisquare_compact_x(d): -298 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) -299 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((d[n_parms + m:].reshape(x_shape) - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) -300 return chisq -301 -302 jac_jac_x = hessian(odr_chisquare_compact_x)(np.concatenate((fitp, out.xplus.ravel(), x_f.ravel()))) +275 number_of_x_parameters = int(m / x_f.shape[-1]) +276 +277 old_jac = jacobian(func)(out.beta, out.xplus) +278 fused_row1 = np.concatenate((old_jac, np.concatenate((number_of_x_parameters * [np.zeros(old_jac.shape)]), axis=0))) +279 fused_row2 = np.concatenate((jacobian(lambda x, y: func(y, x))(out.xplus, out.beta).reshape(x_f.shape[-1], x_f.shape[-1] * number_of_x_parameters), np.identity(number_of_x_parameters * old_jac.shape[0]))) +280 new_jac = np.concatenate((fused_row1, fused_row2), axis=1) +281 +282 A = W @ new_jac +283 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T +284 expected_chisquare = np.trace((np.identity(P_phi.shape[0]) - P_phi) @ W @ cov @ W) +285 if expected_chisquare <= 0.0: +286 warnings.warn("Negative expected_chisquare.", RuntimeWarning) +287 expected_chisquare = np.abs(expected_chisquare) +288 output.chisquare_by_expected_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) / expected_chisquare +289 if not silent: +290 print('chisquare/expected_chisquare:', +291 output.chisquare_by_expected_chisquare) +292 +293 fitp = out.beta +294 try: +295 hess = hessian(odr_chisquare)(np.concatenate((fitp, out.xplus.ravel()))) +296 except TypeError: +297 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None +298 +299 def odr_chisquare_compact_x(d): +300 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) +301 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((d[n_parms + m:].reshape(x_shape) - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) +302 return chisq 303 -304 # Compute hess^{-1} @ jac_jac_x[:n_parms + m, n_parms + m:] using LAPACK dgesv -305 try: -306 deriv_x = -scipy.linalg.solve(hess, jac_jac_x[:n_parms + m, n_parms + m:]) -307 except np.linalg.LinAlgError: -308 raise Exception("Cannot invert hessian matrix.") -309 -310 def odr_chisquare_compact_y(d): -311 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) -312 chisq = anp.sum(((d[n_parms + m:] - model) / dy_f) ** 2) + anp.sum(((x_f - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) -313 return chisq -314 -315 jac_jac_y = hessian(odr_chisquare_compact_y)(np.concatenate((fitp, out.xplus.ravel(), y_f))) +304 jac_jac_x = hessian(odr_chisquare_compact_x)(np.concatenate((fitp, out.xplus.ravel(), x_f.ravel()))) +305 +306 # Compute hess^{-1} @ jac_jac_x[:n_parms + m, n_parms + m:] using LAPACK dgesv +307 try: +308 deriv_x = -scipy.linalg.solve(hess, jac_jac_x[:n_parms + m, n_parms + m:]) +309 except np.linalg.LinAlgError: +310 raise Exception("Cannot invert hessian matrix.") +311 +312 def odr_chisquare_compact_y(d): +313 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) +314 chisq = anp.sum(((d[n_parms + m:] - model) / dy_f) ** 2) + anp.sum(((x_f - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) +315 return chisq 316 -317 # Compute hess^{-1} @ jac_jac_y[:n_parms + m, n_parms + m:] using LAPACK dgesv -318 try: -319 deriv_y = -scipy.linalg.solve(hess, jac_jac_y[:n_parms + m, n_parms + m:]) -320 except np.linalg.LinAlgError: -321 raise Exception("Cannot invert hessian matrix.") -322 -323 result = [] -324 for i in range(n_parms): -325 result.append(derived_observable(lambda my_var, **kwargs: (my_var[0] + np.finfo(np.float64).eps) / (x.ravel()[0].value + np.finfo(np.float64).eps) * out.beta[i], list(x.ravel()) + list(y), man_grad=list(deriv_x[i]) + list(deriv_y[i]))) -326 -327 output.fit_parameters = result +317 jac_jac_y = hessian(odr_chisquare_compact_y)(np.concatenate((fitp, out.xplus.ravel(), y_f))) +318 +319 # Compute hess^{-1} @ jac_jac_y[:n_parms + m, n_parms + m:] using LAPACK dgesv +320 try: +321 deriv_y = -scipy.linalg.solve(hess, jac_jac_y[:n_parms + m, n_parms + m:]) +322 except np.linalg.LinAlgError: +323 raise Exception("Cannot invert hessian matrix.") +324 +325 result = [] +326 for i in range(n_parms): +327 result.append(derived_observable(lambda my_var, **kwargs: (my_var[0] + np.finfo(np.float64).eps) / (x.ravel()[0].value + np.finfo(np.float64).eps) * out.beta[i], list(x.ravel()) + list(y), man_grad=list(deriv_x[i]) + list(deriv_y[i]))) 328 -329 output.odr_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) -330 output.dof = x.shape[-1] - n_parms -331 output.p_value = 1 - scipy.stats.chi2.cdf(output.odr_chisquare, output.dof) -332 -333 return output +329 output.fit_parameters = result +330 +331 output.odr_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) +332 output.dof = x.shape[-1] - n_parms +333 output.p_value = 1 - scipy.stats.chi2.cdf(output.odr_chisquare, output.dof) 334 -335 -336def _prior_fit(x, y, func, priors, silent=False, **kwargs): -337 output = Fit_result() -338 -339 output.fit_function = func +335 return output +336 +337 +338def _prior_fit(x, y, func, priors, silent=False, **kwargs): +339 output = Fit_result() 340 -341 x = np.asarray(x) +341 output.fit_function = func 342 -343 if kwargs.get('num_grad') is True: -344 hessian = num_hessian -345 else: -346 hessian = auto_hessian -347 -348 if not callable(func): -349 raise TypeError('func has to be a function.') -350 -351 for i in range(100): -352 try: -353 func(np.arange(i), 0) -354 except TypeError: -355 continue -356 except IndexError: +343 x = np.asarray(x) +344 +345 if kwargs.get('num_grad') is True: +346 hessian = num_hessian +347 else: +348 hessian = auto_hessian +349 +350 if not callable(func): +351 raise TypeError('func has to be a function.') +352 +353 for i in range(100): +354 try: +355 func(np.arange(i), 0) +356 except TypeError: 357 continue -358 else: -359 break -360 else: -361 raise RuntimeError("Fit function is not valid.") -362 -363 n_parms = i +358 except IndexError: +359 continue +360 else: +361 break +362 else: +363 raise RuntimeError("Fit function is not valid.") 364 -365 if n_parms != len(priors): -366 raise Exception('Priors does not have the correct length.') -367 -368 def extract_val_and_dval(string): -369 split_string = string.split('(') -370 if '.' in split_string[0] and '.' not in split_string[1][:-1]: -371 factor = 10 ** -len(split_string[0].partition('.')[2]) -372 else: -373 factor = 1 -374 return float(split_string[0]), float(split_string[1][:-1]) * factor -375 -376 loc_priors = [] -377 for i_n, i_prior in enumerate(priors): -378 if isinstance(i_prior, Obs): -379 loc_priors.append(i_prior) -380 else: -381 loc_val, loc_dval = extract_val_and_dval(i_prior) -382 loc_priors.append(cov_Obs(loc_val, loc_dval ** 2, '#prior' + str(i_n) + f"_{np.random.randint(2147483647):010d}")) -383 -384 output.priors = loc_priors +365 n_parms = i +366 +367 if n_parms != len(priors): +368 raise Exception('Priors does not have the correct length.') +369 +370 def extract_val_and_dval(string): +371 split_string = string.split('(') +372 if '.' in split_string[0] and '.' not in split_string[1][:-1]: +373 factor = 10 ** -len(split_string[0].partition('.')[2]) +374 else: +375 factor = 1 +376 return float(split_string[0]), float(split_string[1][:-1]) * factor +377 +378 loc_priors = [] +379 for i_n, i_prior in enumerate(priors): +380 if isinstance(i_prior, Obs): +381 loc_priors.append(i_prior) +382 else: +383 loc_val, loc_dval = extract_val_and_dval(i_prior) +384 loc_priors.append(cov_Obs(loc_val, loc_dval ** 2, '#prior' + str(i_n) + f"_{np.random.randint(2147483647):010d}")) 385 -386 if not silent: -387 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) -388 -389 y_f = [o.value for o in y] -390 dy_f = [o.dvalue for o in y] -391 -392 if np.any(np.asarray(dy_f) <= 0.0): -393 raise Exception('No y errors available, run the gamma method first.') -394 -395 p_f = [o.value for o in loc_priors] -396 dp_f = [o.dvalue for o in loc_priors] -397 -398 if np.any(np.asarray(dp_f) <= 0.0): -399 raise Exception('No prior errors available, run the gamma method first.') -400 -401 if 'initial_guess' in kwargs: -402 x0 = kwargs.get('initial_guess') -403 if len(x0) != n_parms: -404 raise Exception('Initial guess does not have the correct length.') -405 else: -406 x0 = p_f -407 -408 def chisqfunc(p): -409 model = func(p, x) -410 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((p_f - p) / dp_f) ** 2) -411 return chisq -412 -413 if not silent: -414 print('Method: migrad') -415 -416 m = iminuit.Minuit(chisqfunc, x0) -417 m.errordef = 1 -418 m.print_level = 0 -419 if 'tol' in kwargs: -420 m.tol = kwargs.get('tol') -421 else: -422 m.tol = 1e-4 -423 m.migrad() -424 params = np.asarray(m.values) -425 -426 output.chisquare_by_dof = m.fval / len(x) +386 output.priors = loc_priors +387 +388 if not silent: +389 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) +390 +391 y_f = [o.value for o in y] +392 dy_f = [o.dvalue for o in y] +393 +394 if np.any(np.asarray(dy_f) <= 0.0): +395 raise Exception('No y errors available, run the gamma method first.') +396 +397 p_f = [o.value for o in loc_priors] +398 dp_f = [o.dvalue for o in loc_priors] +399 +400 if np.any(np.asarray(dp_f) <= 0.0): +401 raise Exception('No prior errors available, run the gamma method first.') +402 +403 if 'initial_guess' in kwargs: +404 x0 = kwargs.get('initial_guess') +405 if len(x0) != n_parms: +406 raise Exception('Initial guess does not have the correct length.') +407 else: +408 x0 = p_f +409 +410 def chisqfunc(p): +411 model = func(p, x) +412 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((p_f - p) / dp_f) ** 2) +413 return chisq +414 +415 if not silent: +416 print('Method: migrad') +417 +418 m = iminuit.Minuit(chisqfunc, x0) +419 m.errordef = 1 +420 m.print_level = 0 +421 if 'tol' in kwargs: +422 m.tol = kwargs.get('tol') +423 else: +424 m.tol = 1e-4 +425 m.migrad() +426 params = np.asarray(m.values) 427 -428 output.method = 'migrad' +428 output.chisquare_by_dof = m.fval / len(x) 429 -430 if not silent: -431 print('chisquare/d.o.f.:', output.chisquare_by_dof) -432 -433 if not m.fmin.is_valid: -434 raise Exception('The minimization procedure did not converge.') -435 -436 hess = hessian(chisqfunc)(params) -437 hess_inv = np.linalg.pinv(hess) -438 -439 def chisqfunc_compact(d): -440 model = func(d[:n_parms], x) -441 chisq = anp.sum(((d[n_parms: n_parms + len(x)] - model) / dy_f) ** 2) + anp.sum(((d[n_parms + len(x):] - d[:n_parms]) / dp_f) ** 2) -442 return chisq -443 -444 jac_jac = hessian(chisqfunc_compact)(np.concatenate((params, y_f, p_f))) +430 output.method = 'migrad' +431 +432 if not silent: +433 print('chisquare/d.o.f.:', output.chisquare_by_dof) +434 +435 if not m.fmin.is_valid: +436 raise Exception('The minimization procedure did not converge.') +437 +438 hess = hessian(chisqfunc)(params) +439 hess_inv = np.linalg.pinv(hess) +440 +441 def chisqfunc_compact(d): +442 model = func(d[:n_parms], x) +443 chisq = anp.sum(((d[n_parms: n_parms + len(x)] - model) / dy_f) ** 2) + anp.sum(((d[n_parms + len(x):] - d[:n_parms]) / dp_f) ** 2) +444 return chisq 445 -446 deriv = -hess_inv @ jac_jac[:n_parms, n_parms:] +446 jac_jac = hessian(chisqfunc_compact)(np.concatenate((params, y_f, p_f))) 447 -448 result = [] -449 for i in range(n_parms): -450 result.append(derived_observable(lambda x, **kwargs: (x[0] + np.finfo(np.float64).eps) / (y[0].value + np.finfo(np.float64).eps) * params[i], list(y) + list(loc_priors), man_grad=list(deriv[i]))) -451 -452 output.fit_parameters = result -453 output.chisquare = chisqfunc(np.asarray(params)) -454 -455 if kwargs.get('resplot') is True: -456 residual_plot(x, y, func, result) -457 -458 if kwargs.get('qqplot') is True: -459 qqplot(x, y, func, result) -460 -461 return output +448 deriv = -hess_inv @ jac_jac[:n_parms, n_parms:] +449 +450 result = [] +451 for i in range(n_parms): +452 result.append(derived_observable(lambda x, **kwargs: (x[0] + np.finfo(np.float64).eps) / (y[0].value + np.finfo(np.float64).eps) * params[i], list(y) + list(loc_priors), man_grad=list(deriv[i]))) +453 +454 output.fit_parameters = result +455 output.chisquare = chisqfunc(np.asarray(params)) +456 +457 if kwargs.get('resplot') is True: +458 residual_plot(x, y, func, result) +459 +460 if kwargs.get('qqplot') is True: +461 qqplot(x, y, func, result) 462 -463 -464def _standard_fit(x, y, func, silent=False, **kwargs): +463 return output +464 465 -466 output = Fit_result() +466def _standard_fit(x, y, func, silent=False, **kwargs): 467 -468 output.fit_function = func +468 output = Fit_result() 469 -470 x = np.asarray(x) +470 output.fit_function = func 471 -472 if kwargs.get('num_grad') is True: -473 jacobian = num_jacobian -474 hessian = num_hessian -475 else: -476 jacobian = auto_jacobian -477 hessian = auto_hessian -478 -479 if x.shape[-1] != len(y): -480 raise Exception('x and y input have to have the same length') -481 -482 if len(x.shape) > 2: -483 raise Exception('Unknown format for x values') -484 -485 if not callable(func): -486 raise TypeError('func has to be a function.') -487 -488 for i in range(42): -489 try: -490 func(np.arange(i), x.T[0]) -491 except TypeError: -492 continue -493 except IndexError: +472 x = np.asarray(x) +473 +474 if kwargs.get('num_grad') is True: +475 jacobian = num_jacobian +476 hessian = num_hessian +477 else: +478 jacobian = auto_jacobian +479 hessian = auto_hessian +480 +481 if x.shape[-1] != len(y): +482 raise Exception('x and y input have to have the same length') +483 +484 if len(x.shape) > 2: +485 raise Exception('Unknown format for x values') +486 +487 if not callable(func): +488 raise TypeError('func has to be a function.') +489 +490 for i in range(42): +491 try: +492 func(np.arange(i), x.T[0]) +493 except TypeError: 494 continue -495 else: -496 break -497 else: -498 raise RuntimeError("Fit function is not valid.") -499 -500 n_parms = i +495 except IndexError: +496 continue +497 else: +498 break +499 else: +500 raise RuntimeError("Fit function is not valid.") 501 -502 if not silent: -503 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) -504 -505 y_f = [o.value for o in y] -506 dy_f = [o.dvalue for o in y] -507 -508 if np.any(np.asarray(dy_f) <= 0.0): -509 raise Exception('No y errors available, run the gamma method first.') -510 -511 if 'initial_guess' in kwargs: -512 x0 = kwargs.get('initial_guess') -513 if len(x0) != n_parms: -514 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) -515 else: -516 x0 = [0.1] * n_parms -517 -518 if kwargs.get('correlated_fit') is True: -519 corr = covariance(y, correlation=True, **kwargs) -520 covdiag = np.diag(1 / np.asarray(dy_f)) -521 condn = np.linalg.cond(corr) -522 if condn > 0.1 / np.finfo(float).eps: -523 raise Exception(f"Cannot invert correlation matrix as its condition number exceeds machine precision ({condn:1.2e})") -524 if condn > 1e13: -525 warnings.warn("Correlation matrix may be ill-conditioned, condition number: {%1.2e}" % (condn), RuntimeWarning) -526 chol = np.linalg.cholesky(corr) -527 chol_inv = scipy.linalg.solve_triangular(chol, covdiag, lower=True) -528 -529 def chisqfunc_corr(p): -530 model = func(p, x) -531 chisq = anp.sum(anp.dot(chol_inv, (y_f - model)) ** 2) -532 return chisq -533 -534 def chisqfunc(p): -535 model = func(p, x) -536 chisq = anp.sum(((y_f - model) / dy_f) ** 2) -537 return chisq -538 -539 output.method = kwargs.get('method', 'Levenberg-Marquardt') -540 if not silent: -541 print('Method:', output.method) -542 -543 if output.method != 'Levenberg-Marquardt': -544 if output.method == 'migrad': -545 fit_result = iminuit.minimize(chisqfunc, x0, tol=1e-4) # Stopping criterion 0.002 * tol * errordef -546 if kwargs.get('correlated_fit') is True: -547 fit_result = iminuit.minimize(chisqfunc_corr, fit_result.x, tol=1e-4) # Stopping criterion 0.002 * tol * errordef -548 output.iterations = fit_result.nfev -549 else: -550 fit_result = scipy.optimize.minimize(chisqfunc, x0, method=kwargs.get('method'), tol=1e-12) -551 if kwargs.get('correlated_fit') is True: -552 fit_result = scipy.optimize.minimize(chisqfunc_corr, fit_result.x, method=kwargs.get('method'), tol=1e-12) -553 output.iterations = fit_result.nit -554 -555 chisquare = fit_result.fun +502 n_parms = i +503 +504 if not silent: +505 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) +506 +507 y_f = [o.value for o in y] +508 dy_f = [o.dvalue for o in y] +509 +510 if np.any(np.asarray(dy_f) <= 0.0): +511 raise Exception('No y errors available, run the gamma method first.') +512 +513 if 'initial_guess' in kwargs: +514 x0 = kwargs.get('initial_guess') +515 if len(x0) != n_parms: +516 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) +517 else: +518 x0 = [0.1] * n_parms +519 +520 if kwargs.get('correlated_fit') is True: +521 corr = covariance(y, correlation=True, **kwargs) +522 covdiag = np.diag(1 / np.asarray(dy_f)) +523 condn = np.linalg.cond(corr) +524 if condn > 0.1 / np.finfo(float).eps: +525 raise Exception(f"Cannot invert correlation matrix as its condition number exceeds machine precision ({condn:1.2e})") +526 if condn > 1e13: +527 warnings.warn("Correlation matrix may be ill-conditioned, condition number: {%1.2e}" % (condn), RuntimeWarning) +528 chol = np.linalg.cholesky(corr) +529 chol_inv = scipy.linalg.solve_triangular(chol, covdiag, lower=True) +530 +531 def chisqfunc_corr(p): +532 model = func(p, x) +533 chisq = anp.sum(anp.dot(chol_inv, (y_f - model)) ** 2) +534 return chisq +535 +536 def chisqfunc(p): +537 model = func(p, x) +538 chisq = anp.sum(((y_f - model) / dy_f) ** 2) +539 return chisq +540 +541 output.method = kwargs.get('method', 'Levenberg-Marquardt') +542 if not silent: +543 print('Method:', output.method) +544 +545 if output.method != 'Levenberg-Marquardt': +546 if output.method == 'migrad': +547 fit_result = iminuit.minimize(chisqfunc, x0, tol=1e-4) # Stopping criterion 0.002 * tol * errordef +548 if kwargs.get('correlated_fit') is True: +549 fit_result = iminuit.minimize(chisqfunc_corr, fit_result.x, tol=1e-4) # Stopping criterion 0.002 * tol * errordef +550 output.iterations = fit_result.nfev +551 else: +552 fit_result = scipy.optimize.minimize(chisqfunc, x0, method=kwargs.get('method'), tol=1e-12) +553 if kwargs.get('correlated_fit') is True: +554 fit_result = scipy.optimize.minimize(chisqfunc_corr, fit_result.x, method=kwargs.get('method'), tol=1e-12) +555 output.iterations = fit_result.nit 556 -557 else: -558 if kwargs.get('correlated_fit') is True: -559 def chisqfunc_residuals_corr(p): -560 model = func(p, x) -561 chisq = anp.dot(chol_inv, (y_f - model)) -562 return chisq -563 -564 def chisqfunc_residuals(p): -565 model = func(p, x) -566 chisq = ((y_f - model) / dy_f) -567 return chisq -568 -569 fit_result = scipy.optimize.least_squares(chisqfunc_residuals, x0, method='lm', ftol=1e-15, gtol=1e-15, xtol=1e-15) -570 if kwargs.get('correlated_fit') is True: -571 fit_result = scipy.optimize.least_squares(chisqfunc_residuals_corr, fit_result.x, method='lm', ftol=1e-15, gtol=1e-15, xtol=1e-15) -572 -573 chisquare = np.sum(fit_result.fun ** 2) -574 if kwargs.get('correlated_fit') is True: -575 assert np.isclose(chisquare, chisqfunc_corr(fit_result.x), atol=1e-14) -576 else: -577 assert np.isclose(chisquare, chisqfunc(fit_result.x), atol=1e-14) -578 -579 output.iterations = fit_result.nfev +557 chisquare = fit_result.fun +558 +559 else: +560 if kwargs.get('correlated_fit') is True: +561 def chisqfunc_residuals_corr(p): +562 model = func(p, x) +563 chisq = anp.dot(chol_inv, (y_f - model)) +564 return chisq +565 +566 def chisqfunc_residuals(p): +567 model = func(p, x) +568 chisq = ((y_f - model) / dy_f) +569 return chisq +570 +571 fit_result = scipy.optimize.least_squares(chisqfunc_residuals, x0, method='lm', ftol=1e-15, gtol=1e-15, xtol=1e-15) +572 if kwargs.get('correlated_fit') is True: +573 fit_result = scipy.optimize.least_squares(chisqfunc_residuals_corr, fit_result.x, method='lm', ftol=1e-15, gtol=1e-15, xtol=1e-15) +574 +575 chisquare = np.sum(fit_result.fun ** 2) +576 if kwargs.get('correlated_fit') is True: +577 assert np.isclose(chisquare, chisqfunc_corr(fit_result.x), atol=1e-14) +578 else: +579 assert np.isclose(chisquare, chisqfunc(fit_result.x), atol=1e-14) 580 -581 if not fit_result.success: -582 raise Exception('The minimization procedure did not converge.') -583 -584 if x.shape[-1] - n_parms > 0: -585 output.chisquare_by_dof = chisquare / (x.shape[-1] - n_parms) -586 else: -587 output.chisquare_by_dof = float('nan') -588 -589 output.message = fit_result.message -590 if not silent: -591 print(fit_result.message) -592 print('chisquare/d.o.f.:', output.chisquare_by_dof) -593 -594 if kwargs.get('expected_chisquare') is True: -595 if kwargs.get('correlated_fit') is not True: -596 W = np.diag(1 / np.asarray(dy_f)) -597 cov = covariance(y) -598 A = W @ jacobian(func)(fit_result.x, x) -599 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T -600 expected_chisquare = np.trace((np.identity(x.shape[-1]) - P_phi) @ W @ cov @ W) -601 output.chisquare_by_expected_chisquare = chisquare / expected_chisquare -602 if not silent: -603 print('chisquare/expected_chisquare:', -604 output.chisquare_by_expected_chisquare) -605 -606 fitp = fit_result.x -607 try: -608 if kwargs.get('correlated_fit') is True: -609 hess = hessian(chisqfunc_corr)(fitp) -610 else: -611 hess = hessian(chisqfunc)(fitp) -612 except TypeError: -613 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None -614 -615 if kwargs.get('correlated_fit') is True: -616 def chisqfunc_compact(d): -617 model = func(d[:n_parms], x) -618 chisq = anp.sum(anp.dot(chol_inv, (d[n_parms:] - model)) ** 2) -619 return chisq -620 -621 else: -622 def chisqfunc_compact(d): -623 model = func(d[:n_parms], x) -624 chisq = anp.sum(((d[n_parms:] - model) / dy_f) ** 2) -625 return chisq -626 -627 jac_jac = hessian(chisqfunc_compact)(np.concatenate((fitp, y_f))) +581 output.iterations = fit_result.nfev +582 +583 if not fit_result.success: +584 raise Exception('The minimization procedure did not converge.') +585 +586 if x.shape[-1] - n_parms > 0: +587 output.chisquare_by_dof = chisquare / (x.shape[-1] - n_parms) +588 else: +589 output.chisquare_by_dof = float('nan') +590 +591 output.message = fit_result.message +592 if not silent: +593 print(fit_result.message) +594 print('chisquare/d.o.f.:', output.chisquare_by_dof) +595 +596 if kwargs.get('expected_chisquare') is True: +597 if kwargs.get('correlated_fit') is not True: +598 W = np.diag(1 / np.asarray(dy_f)) +599 cov = covariance(y) +600 A = W @ jacobian(func)(fit_result.x, x) +601 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T +602 expected_chisquare = np.trace((np.identity(x.shape[-1]) - P_phi) @ W @ cov @ W) +603 output.chisquare_by_expected_chisquare = chisquare / expected_chisquare +604 if not silent: +605 print('chisquare/expected_chisquare:', +606 output.chisquare_by_expected_chisquare) +607 +608 fitp = fit_result.x +609 try: +610 if kwargs.get('correlated_fit') is True: +611 hess = hessian(chisqfunc_corr)(fitp) +612 else: +613 hess = hessian(chisqfunc)(fitp) +614 except TypeError: +615 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None +616 +617 if kwargs.get('correlated_fit') is True: +618 def chisqfunc_compact(d): +619 model = func(d[:n_parms], x) +620 chisq = anp.sum(anp.dot(chol_inv, (d[n_parms:] - model)) ** 2) +621 return chisq +622 +623 else: +624 def chisqfunc_compact(d): +625 model = func(d[:n_parms], x) +626 chisq = anp.sum(((d[n_parms:] - model) / dy_f) ** 2) +627 return chisq 628 -629 # Compute hess^{-1} @ jac_jac[:n_parms, n_parms:] using LAPACK dgesv -630 try: -631 deriv = -scipy.linalg.solve(hess, jac_jac[:n_parms, n_parms:]) -632 except np.linalg.LinAlgError: -633 raise Exception("Cannot invert hessian matrix.") -634 -635 result = [] -636 for i in range(n_parms): -637 result.append(derived_observable(lambda x, **kwargs: (x[0] + np.finfo(np.float64).eps) / (y[0].value + np.finfo(np.float64).eps) * fit_result.x[i], list(y), man_grad=list(deriv[i]))) -638 -639 output.fit_parameters = result +629 jac_jac = hessian(chisqfunc_compact)(np.concatenate((fitp, y_f))) +630 +631 # Compute hess^{-1} @ jac_jac[:n_parms, n_parms:] using LAPACK dgesv +632 try: +633 deriv = -scipy.linalg.solve(hess, jac_jac[:n_parms, n_parms:]) +634 except np.linalg.LinAlgError: +635 raise Exception("Cannot invert hessian matrix.") +636 +637 result = [] +638 for i in range(n_parms): +639 result.append(derived_observable(lambda x, **kwargs: (x[0] + np.finfo(np.float64).eps) / (y[0].value + np.finfo(np.float64).eps) * fit_result.x[i], list(y), man_grad=list(deriv[i]))) 640 -641 output.chisquare = chisquare -642 output.dof = x.shape[-1] - n_parms -643 output.p_value = 1 - scipy.stats.chi2.cdf(output.chisquare, output.dof) -644 # Hotelling t-squared p-value for correlated fits. -645 if kwargs.get('correlated_fit') is True: -646 n_cov = np.min(np.vectorize(lambda x: x.N)(y)) -647 output.t2_p_value = 1 - scipy.stats.f.cdf((n_cov - output.dof) / (output.dof * (n_cov - 1)) * output.chisquare, -648 output.dof, n_cov - output.dof) -649 -650 if kwargs.get('resplot') is True: -651 residual_plot(x, y, func, result) -652 -653 if kwargs.get('qqplot') is True: -654 qqplot(x, y, func, result) -655 -656 return output +641 output.fit_parameters = result +642 +643 output.chisquare = chisquare +644 output.dof = x.shape[-1] - n_parms +645 output.p_value = 1 - scipy.stats.chi2.cdf(output.chisquare, output.dof) +646 # Hotelling t-squared p-value for correlated fits. +647 if kwargs.get('correlated_fit') is True: +648 n_cov = np.min(np.vectorize(lambda x: x.N)(y)) +649 output.t2_p_value = 1 - scipy.stats.f.cdf((n_cov - output.dof) / (output.dof * (n_cov - 1)) * output.chisquare, +650 output.dof, n_cov - output.dof) +651 +652 if kwargs.get('resplot') is True: +653 residual_plot(x, y, func, result) +654 +655 if kwargs.get('qqplot') is True: +656 qqplot(x, y, func, result) 657 -658 -659def fit_lin(x, y, **kwargs): -660 """Performs a linear fit to y = n + m * x and returns two Obs n, m. -661 -662 Parameters -663 ---------- -664 x : list -665 Can either be a list of floats in which case no xerror is assumed, or -666 a list of Obs, where the dvalues of the Obs are used as xerror for the fit. -667 y : list -668 List of Obs, the dvalues of the Obs are used as yerror for the fit. -669 """ -670 -671 def f(a, x): -672 y = a[0] + a[1] * x -673 return y -674 -675 if all(isinstance(n, Obs) for n in x): -676 out = total_least_squares(x, y, f, **kwargs) -677 return out.fit_parameters -678 elif all(isinstance(n, float) or isinstance(n, int) for n in x) or isinstance(x, np.ndarray): -679 out = least_squares(x, y, f, **kwargs) -680 return out.fit_parameters -681 else: -682 raise Exception('Unsupported types for x') -683 -684 -685def qqplot(x, o_y, func, p): -686 """Generates a quantile-quantile plot of the fit result which can be used to -687 check if the residuals of the fit are gaussian distributed. -688 """ -689 -690 residuals = [] -691 for i_x, i_y in zip(x, o_y): -692 residuals.append((i_y - func(p, i_x)) / i_y.dvalue) -693 residuals = sorted(residuals) -694 my_y = [o.value for o in residuals] -695 probplot = scipy.stats.probplot(my_y) -696 my_x = probplot[0][0] -697 plt.figure(figsize=(8, 8 / 1.618)) -698 plt.errorbar(my_x, my_y, fmt='o') -699 fit_start = my_x[0] -700 fit_stop = my_x[-1] -701 samples = np.arange(fit_start, fit_stop, 0.01) -702 plt.plot(samples, samples, 'k--', zorder=11, label='Standard normal distribution') -703 plt.plot(samples, probplot[1][0] * samples + probplot[1][1], zorder=10, label='Least squares fit, r=' + str(np.around(probplot[1][2], 3)), marker='', ls='-') -704 -705 plt.xlabel('Theoretical quantiles') -706 plt.ylabel('Ordered Values') -707 plt.legend() -708 plt.draw() -709 -710 -711def residual_plot(x, y, func, fit_res): -712 """ Generates a plot which compares the fit to the data and displays the corresponding residuals""" -713 sorted_x = sorted(x) -714 xstart = sorted_x[0] - 0.5 * (sorted_x[1] - sorted_x[0]) -715 xstop = sorted_x[-1] + 0.5 * (sorted_x[-1] - sorted_x[-2]) -716 x_samples = np.arange(xstart, xstop + 0.01, 0.01) -717 -718 plt.figure(figsize=(8, 8 / 1.618)) -719 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) -720 ax0 = plt.subplot(gs[0]) -721 ax0.errorbar(x, [o.value for o in y], yerr=[o.dvalue for o in y], ls='none', fmt='o', capsize=3, markersize=5, label='Data') -722 ax0.plot(x_samples, func([o.value for o in fit_res], x_samples), label='Fit', zorder=10, ls='-', ms=0) -723 ax0.set_xticklabels([]) -724 ax0.set_xlim([xstart, xstop]) +658 return output +659 +660 +661def fit_lin(x, y, **kwargs): +662 """Performs a linear fit to y = n + m * x and returns two Obs n, m. +663 +664 Parameters +665 ---------- +666 x : list +667 Can either be a list of floats in which case no xerror is assumed, or +668 a list of Obs, where the dvalues of the Obs are used as xerror for the fit. +669 y : list +670 List of Obs, the dvalues of the Obs are used as yerror for the fit. +671 """ +672 +673 def f(a, x): +674 y = a[0] + a[1] * x +675 return y +676 +677 if all(isinstance(n, Obs) for n in x): +678 out = total_least_squares(x, y, f, **kwargs) +679 return out.fit_parameters +680 elif all(isinstance(n, float) or isinstance(n, int) for n in x) or isinstance(x, np.ndarray): +681 out = least_squares(x, y, f, **kwargs) +682 return out.fit_parameters +683 else: +684 raise Exception('Unsupported types for x') +685 +686 +687def qqplot(x, o_y, func, p): +688 """Generates a quantile-quantile plot of the fit result which can be used to +689 check if the residuals of the fit are gaussian distributed. +690 """ +691 +692 residuals = [] +693 for i_x, i_y in zip(x, o_y): +694 residuals.append((i_y - func(p, i_x)) / i_y.dvalue) +695 residuals = sorted(residuals) +696 my_y = [o.value for o in residuals] +697 probplot = scipy.stats.probplot(my_y) +698 my_x = probplot[0][0] +699 plt.figure(figsize=(8, 8 / 1.618)) +700 plt.errorbar(my_x, my_y, fmt='o') +701 fit_start = my_x[0] +702 fit_stop = my_x[-1] +703 samples = np.arange(fit_start, fit_stop, 0.01) +704 plt.plot(samples, samples, 'k--', zorder=11, label='Standard normal distribution') +705 plt.plot(samples, probplot[1][0] * samples + probplot[1][1], zorder=10, label='Least squares fit, r=' + str(np.around(probplot[1][2], 3)), marker='', ls='-') +706 +707 plt.xlabel('Theoretical quantiles') +708 plt.ylabel('Ordered Values') +709 plt.legend() +710 plt.draw() +711 +712 +713def residual_plot(x, y, func, fit_res): +714 """ Generates a plot which compares the fit to the data and displays the corresponding residuals""" +715 sorted_x = sorted(x) +716 xstart = sorted_x[0] - 0.5 * (sorted_x[1] - sorted_x[0]) +717 xstop = sorted_x[-1] + 0.5 * (sorted_x[-1] - sorted_x[-2]) +718 x_samples = np.arange(xstart, xstop + 0.01, 0.01) +719 +720 plt.figure(figsize=(8, 8 / 1.618)) +721 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) +722 ax0 = plt.subplot(gs[0]) +723 ax0.errorbar(x, [o.value for o in y], yerr=[o.dvalue for o in y], ls='none', fmt='o', capsize=3, markersize=5, label='Data') +724 ax0.plot(x_samples, func([o.value for o in fit_res], x_samples), label='Fit', zorder=10, ls='-', ms=0) 725 ax0.set_xticklabels([]) -726 ax0.legend() -727 -728 residuals = (np.asarray([o.value for o in y]) - func([o.value for o in fit_res], x)) / np.asarray([o.dvalue for o in y]) -729 ax1 = plt.subplot(gs[1]) -730 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) -731 ax1.tick_params(direction='out') -732 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) -733 ax1.axhline(y=0.0, ls='--', color='k', marker=" ") -734 ax1.fill_between(x_samples, -1.0, 1.0, alpha=0.1, facecolor='k') -735 ax1.set_xlim([xstart, xstop]) -736 ax1.set_ylabel('Residuals') -737 plt.subplots_adjust(wspace=None, hspace=None) -738 plt.draw() -739 -740 -741def error_band(x, func, beta): -742 """Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.""" -743 cov = covariance(beta) -744 if np.any(np.abs(cov - cov.T) > 1000 * np.finfo(np.float64).eps): -745 warnings.warn("Covariance matrix is not symmetric within floating point precision", RuntimeWarning) -746 -747 deriv = [] -748 for i, item in enumerate(x): -749 deriv.append(np.array(egrad(func)([o.value for o in beta], item))) -750 -751 err = [] -752 for i, item in enumerate(x): -753 err.append(np.sqrt(deriv[i] @ cov @ deriv[i])) -754 err = np.array(err) -755 -756 return err +726 ax0.set_xlim([xstart, xstop]) +727 ax0.set_xticklabels([]) +728 ax0.legend() +729 +730 residuals = (np.asarray([o.value for o in y]) - func([o.value for o in fit_res], x)) / np.asarray([o.dvalue for o in y]) +731 ax1 = plt.subplot(gs[1]) +732 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) +733 ax1.tick_params(direction='out') +734 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) +735 ax1.axhline(y=0.0, ls='--', color='k', marker=" ") +736 ax1.fill_between(x_samples, -1.0, 1.0, alpha=0.1, facecolor='k') +737 ax1.set_xlim([xstart, xstop]) +738 ax1.set_ylabel('Residuals') +739 plt.subplots_adjust(wspace=None, hspace=None) +740 plt.draw() +741 +742 +743def error_band(x, func, beta): +744 """Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.""" +745 cov = covariance(beta) +746 if np.any(np.abs(cov - cov.T) > 1000 * np.finfo(np.float64).eps): +747 warnings.warn("Covariance matrix is not symmetric within floating point precision", RuntimeWarning) +748 +749 deriv = [] +750 for i, item in enumerate(x): +751 deriv.append(np.array(egrad(func)([o.value for o in beta], item))) +752 +753 err = [] +754 for i, item in enumerate(x): +755 err.append(np.sqrt(deriv[i] @ cov @ deriv[i])) +756 err = np.array(err) 757 -758 -759def ks_test(objects=None): -760 """Performs a Kolmogorov–Smirnov test for the p-values of all fit object. -761 -762 Parameters -763 ---------- -764 objects : list -765 List of fit results to include in the analysis (optional). -766 """ -767 -768 if objects is None: -769 obs_list = [] -770 for obj in gc.get_objects(): -771 if isinstance(obj, Fit_result): -772 obs_list.append(obj) -773 else: -774 obs_list = objects -775 -776 p_values = [o.p_value for o in obs_list] +758 return err +759 +760 +761def ks_test(objects=None): +762 """Performs a Kolmogorov–Smirnov test for the p-values of all fit object. +763 +764 Parameters +765 ---------- +766 objects : list +767 List of fit results to include in the analysis (optional). +768 """ +769 +770 if objects is None: +771 obs_list = [] +772 for obj in gc.get_objects(): +773 if isinstance(obj, Fit_result): +774 obs_list.append(obj) +775 else: +776 obs_list = objects 777 -778 bins = len(p_values) -779 x = np.arange(0, 1.001, 0.001) -780 plt.plot(x, x, 'k', zorder=1) -781 plt.xlim(0, 1) -782 plt.ylim(0, 1) -783 plt.xlabel('p-value') -784 plt.ylabel('Cumulative probability') -785 plt.title(str(bins) + ' p-values') -786 -787 n = np.arange(1, bins + 1) / np.float64(bins) -788 Xs = np.sort(p_values) -789 plt.step(Xs, n) -790 diffs = n - Xs -791 loc_max_diff = np.argmax(np.abs(diffs)) -792 loc = Xs[loc_max_diff] -793 plt.annotate('', xy=(loc, loc), xytext=(loc, loc + diffs[loc_max_diff]), arrowprops=dict(arrowstyle='<->', shrinkA=0, shrinkB=0)) -794 plt.draw() -795 -796 print(scipy.stats.kstest(p_values, 'uniform')) +778 p_values = [o.p_value for o in obs_list] +779 +780 bins = len(p_values) +781 x = np.arange(0, 1.001, 0.001) +782 plt.plot(x, x, 'k', zorder=1) +783 plt.xlim(0, 1) +784 plt.ylim(0, 1) +785 plt.xlabel('p-value') +786 plt.ylabel('Cumulative probability') +787 plt.title(str(bins) + ' p-values') +788 +789 n = np.arange(1, bins + 1) / np.float64(bins) +790 Xs = np.sort(p_values) +791 plt.step(Xs, n) +792 diffs = n - Xs +793 loc_max_diff = np.argmax(np.abs(diffs)) +794 loc = Xs[loc_max_diff] +795 plt.annotate('', xy=(loc, loc), xytext=(loc, loc + diffs[loc_max_diff]), arrowprops=dict(arrowstyle='<->', shrinkA=0, shrinkB=0)) +796 plt.draw() +797 +798 print(scipy.stats.kstest(p_values, 'uniform'))
Apply the gamma method to all fit parameters
+46 def gamma_method(self, **kwargs): +47 """Apply the gamma method to all fit parameters""" +48 [o.gamma_method(**kwargs) for o in self.fit_parameters] +
Apply the gamma method to all fit parameters
72def least_squares(x, y, func, priors=None, silent=False, **kwargs): - 73 r'''Performs a non-linear fit to y = func(x). - 74 - 75 Parameters - 76 ---------- - 77 x : list - 78 list of floats. - 79 y : list - 80 list of Obs. - 81 func : object - 82 fit function, has to be of the form - 83 - 84 ```python - 85 import autograd.numpy as anp - 86 - 87 def func(a, x): - 88 return a[0] + a[1] * x + a[2] * anp.sinh(x) - 89 ``` - 90 - 91 For multiple x values func can be of the form +@@ -1193,203 +1222,203 @@ Use numerical differentation instead of automatic differentiation to perform the74def least_squares(x, y, func, priors=None, silent=False, **kwargs): + 75 r'''Performs a non-linear fit to y = func(x). + 76 + 77 Parameters + 78 ---------- + 79 x : list + 80 list of floats. + 81 y : list + 82 list of Obs. + 83 func : object + 84 fit function, has to be of the form + 85 + 86 ```python + 87 import autograd.numpy as anp + 88 + 89 def func(a, x): + 90 return a[0] + a[1] * x + a[2] * anp.sinh(x) + 91 ``` 92 - 93 ```python - 94 def func(a, x): - 95 (x1, x2) = x - 96 return a[0] * x1 ** 2 + a[1] * x2 - 97 ``` - 98 - 99 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation -100 will not work. -101 priors : list, optional -102 priors has to be a list with an entry for every parameter in the fit. The entries can either be -103 Obs (e.g. results from a previous fit) or strings containing a value and an error formatted like -104 0.548(23), 500(40) or 0.5(0.4) -105 silent : bool, optional -106 If true all output to the console is omitted (default False). -107 initial_guess : list -108 can provide an initial guess for the input parameters. Relevant for -109 non-linear fits with many parameters. In case of correlated fits the guess is used to perform -110 an uncorrelated fit which then serves as guess for the correlated fit. -111 method : str, optional -112 can be used to choose an alternative method for the minimization of chisquare. -113 The possible methods are the ones which can be used for scipy.optimize.minimize and -114 migrad of iminuit. If no method is specified, Levenberg-Marquard is used. -115 Reliable alternatives are migrad, Powell and Nelder-Mead. -116 correlated_fit : bool -117 If True, use the full inverse covariance matrix in the definition of the chisquare cost function. -118 For details about how the covariance matrix is estimated see `pyerrors.obs.covariance`. -119 In practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix). -120 This procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning). -121 At the moment this option only works for `prior==None` and when no `method` is given. -122 expected_chisquare : bool -123 If True estimates the expected chisquare which is -124 corrected by effects caused by correlated input data (default False). -125 resplot : bool -126 If True, a plot which displays fit, data and residuals is generated (default False). -127 qqplot : bool -128 If True, a quantile-quantile plot of the fit result is generated (default False). -129 num_grad : bool -130 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). -131 ''' -132 if priors is not None: -133 return _prior_fit(x, y, func, priors, silent=silent, **kwargs) -134 else: -135 return _standard_fit(x, y, func, silent=silent, **kwargs) + 93 For multiple x values func can be of the form + 94 + 95 ```python + 96 def func(a, x): + 97 (x1, x2) = x + 98 return a[0] * x1 ** 2 + a[1] * x2 + 99 ``` +100 +101 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation +102 will not work. +103 priors : list, optional +104 priors has to be a list with an entry for every parameter in the fit. The entries can either be +105 Obs (e.g. results from a previous fit) or strings containing a value and an error formatted like +106 0.548(23), 500(40) or 0.5(0.4) +107 silent : bool, optional +108 If true all output to the console is omitted (default False). +109 initial_guess : list +110 can provide an initial guess for the input parameters. Relevant for +111 non-linear fits with many parameters. In case of correlated fits the guess is used to perform +112 an uncorrelated fit which then serves as guess for the correlated fit. +113 method : str, optional +114 can be used to choose an alternative method for the minimization of chisquare. +115 The possible methods are the ones which can be used for scipy.optimize.minimize and +116 migrad of iminuit. If no method is specified, Levenberg-Marquard is used. +117 Reliable alternatives are migrad, Powell and Nelder-Mead. +118 correlated_fit : bool +119 If True, use the full inverse covariance matrix in the definition of the chisquare cost function. +120 For details about how the covariance matrix is estimated see `pyerrors.obs.covariance`. +121 In practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix). +122 This procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning). +123 At the moment this option only works for `prior==None` and when no `method` is given. +124 expected_chisquare : bool +125 If True estimates the expected chisquare which is +126 corrected by effects caused by correlated input data (default False). +127 resplot : bool +128 If True, a plot which displays fit, data and residuals is generated (default False). +129 qqplot : bool +130 If True, a quantile-quantile plot of the fit result is generated (default False). +131 num_grad : bool +132 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). +133 ''' +134 if priors is not None: +135 return _prior_fit(x, y, func, priors, silent=silent, **kwargs) +136 else: +137 return _standard_fit(x, y, func, silent=silent, **kwargs)
138def total_least_squares(x, y, func, silent=False, **kwargs): -139 r'''Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters. -140 -141 Parameters -142 ---------- -143 x : list -144 list of Obs, or a tuple of lists of Obs -145 y : list -146 list of Obs. The dvalues of the Obs are used as x- and yerror for the fit. -147 func : object -148 func has to be of the form -149 -150 ```python -151 import autograd.numpy as anp -152 -153 def func(a, x): -154 return a[0] + a[1] * x + a[2] * anp.sinh(x) -155 ``` -156 -157 For multiple x values func can be of the form +@@ -1456,30 +1485,30 @@ Use numerical differentation instead of automatic differentiation to perform the140def total_least_squares(x, y, func, silent=False, **kwargs): +141 r'''Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters. +142 +143 Parameters +144 ---------- +145 x : list +146 list of Obs, or a tuple of lists of Obs +147 y : list +148 list of Obs. The dvalues of the Obs are used as x- and yerror for the fit. +149 func : object +150 func has to be of the form +151 +152 ```python +153 import autograd.numpy as anp +154 +155 def func(a, x): +156 return a[0] + a[1] * x + a[2] * anp.sinh(x) +157 ``` 158 -159 ```python -160 def func(a, x): -161 (x1, x2) = x -162 return a[0] * x1 ** 2 + a[1] * x2 -163 ``` -164 -165 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation -166 will not work. -167 silent : bool, optional -168 If true all output to the console is omitted (default False). -169 initial_guess : list -170 can provide an initial guess for the input parameters. Relevant for non-linear -171 fits with many parameters. -172 expected_chisquare : bool -173 If true prints the expected chisquare which is -174 corrected by effects caused by correlated input data. -175 This can take a while as the full correlation matrix -176 has to be calculated (default False). -177 num_grad : bool -178 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). -179 -180 Notes -181 ----- -182 Based on the orthogonal distance regression module of scipy -183 ''' -184 -185 output = Fit_result() +159 For multiple x values func can be of the form +160 +161 ```python +162 def func(a, x): +163 (x1, x2) = x +164 return a[0] * x1 ** 2 + a[1] * x2 +165 ``` +166 +167 It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation +168 will not work. +169 silent : bool, optional +170 If true all output to the console is omitted (default False). +171 initial_guess : list +172 can provide an initial guess for the input parameters. Relevant for non-linear +173 fits with many parameters. +174 expected_chisquare : bool +175 If true prints the expected chisquare which is +176 corrected by effects caused by correlated input data. +177 This can take a while as the full correlation matrix +178 has to be calculated (default False). +179 num_grad : bool +180 Use numerical differentation instead of automatic differentiation to perform the error propagation (default False). +181 +182 Notes +183 ----- +184 Based on the orthogonal distance regression module of scipy +185 ''' 186 -187 output.fit_function = func +187 output = Fit_result() 188 -189 x = np.array(x) +189 output.fit_function = func 190 -191 x_shape = x.shape +191 x = np.array(x) 192 -193 if kwargs.get('num_grad') is True: -194 jacobian = num_jacobian -195 hessian = num_hessian -196 else: -197 jacobian = auto_jacobian -198 hessian = auto_hessian -199 -200 if not callable(func): -201 raise TypeError('func has to be a function.') -202 -203 for i in range(42): -204 try: -205 func(np.arange(i), x.T[0]) -206 except TypeError: -207 continue -208 except IndexError: +193 x_shape = x.shape +194 +195 if kwargs.get('num_grad') is True: +196 jacobian = num_jacobian +197 hessian = num_hessian +198 else: +199 jacobian = auto_jacobian +200 hessian = auto_hessian +201 +202 if not callable(func): +203 raise TypeError('func has to be a function.') +204 +205 for i in range(42): +206 try: +207 func(np.arange(i), x.T[0]) +208 except TypeError: 209 continue -210 else: -211 break -212 else: -213 raise RuntimeError("Fit function is not valid.") -214 -215 n_parms = i -216 if not silent: -217 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) -218 -219 x_f = np.vectorize(lambda o: o.value)(x) -220 dx_f = np.vectorize(lambda o: o.dvalue)(x) -221 y_f = np.array([o.value for o in y]) -222 dy_f = np.array([o.dvalue for o in y]) -223 -224 if np.any(np.asarray(dx_f) <= 0.0): -225 raise Exception('No x errors available, run the gamma method first.') -226 -227 if np.any(np.asarray(dy_f) <= 0.0): -228 raise Exception('No y errors available, run the gamma method first.') -229 -230 if 'initial_guess' in kwargs: -231 x0 = kwargs.get('initial_guess') -232 if len(x0) != n_parms: -233 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) -234 else: -235 x0 = [1] * n_parms -236 -237 data = RealData(x_f, y_f, sx=dx_f, sy=dy_f) -238 model = Model(func) -239 odr = ODR(data, model, x0, partol=np.finfo(np.float64).eps) -240 odr.set_job(fit_type=0, deriv=1) -241 out = odr.run() -242 -243 output.residual_variance = out.res_var +210 except IndexError: +211 continue +212 else: +213 break +214 else: +215 raise RuntimeError("Fit function is not valid.") +216 +217 n_parms = i +218 if not silent: +219 print('Fit with', n_parms, 'parameter' + 's' * (n_parms > 1)) +220 +221 x_f = np.vectorize(lambda o: o.value)(x) +222 dx_f = np.vectorize(lambda o: o.dvalue)(x) +223 y_f = np.array([o.value for o in y]) +224 dy_f = np.array([o.dvalue for o in y]) +225 +226 if np.any(np.asarray(dx_f) <= 0.0): +227 raise Exception('No x errors available, run the gamma method first.') +228 +229 if np.any(np.asarray(dy_f) <= 0.0): +230 raise Exception('No y errors available, run the gamma method first.') +231 +232 if 'initial_guess' in kwargs: +233 x0 = kwargs.get('initial_guess') +234 if len(x0) != n_parms: +235 raise Exception('Initial guess does not have the correct length: %d vs. %d' % (len(x0), n_parms)) +236 else: +237 x0 = [1] * n_parms +238 +239 data = RealData(x_f, y_f, sx=dx_f, sy=dy_f) +240 model = Model(func) +241 odr = ODR(data, model, x0, partol=np.finfo(np.float64).eps) +242 odr.set_job(fit_type=0, deriv=1) +243 out = odr.run() 244 -245 output.method = 'ODR' +245 output.residual_variance = out.res_var 246 -247 output.message = out.stopreason +247 output.method = 'ODR' 248 -249 output.xplus = out.xplus +249 output.message = out.stopreason 250 -251 if not silent: -252 print('Method: ODR') -253 print(*out.stopreason) -254 print('Residual variance:', output.residual_variance) -255 -256 if out.info > 3: -257 raise Exception('The minimization procedure did not converge.') -258 -259 m = x_f.size +251 output.xplus = out.xplus +252 +253 if not silent: +254 print('Method: ODR') +255 print(*out.stopreason) +256 print('Residual variance:', output.residual_variance) +257 +258 if out.info > 3: +259 raise Exception('The minimization procedure did not converge.') 260 -261 def odr_chisquare(p): -262 model = func(p[:n_parms], p[n_parms:].reshape(x_shape)) -263 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((x_f - p[n_parms:].reshape(x_shape)) / dx_f) ** 2) -264 return chisq -265 -266 if kwargs.get('expected_chisquare') is True: -267 W = np.diag(1 / np.asarray(np.concatenate((dy_f.ravel(), dx_f.ravel())))) -268 -269 if kwargs.get('covariance') is not None: -270 cov = kwargs.get('covariance') -271 else: -272 cov = covariance(np.concatenate((y, x.ravel()))) -273 -274 number_of_x_parameters = int(m / x_f.shape[-1]) +261 m = x_f.size +262 +263 def odr_chisquare(p): +264 model = func(p[:n_parms], p[n_parms:].reshape(x_shape)) +265 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((x_f - p[n_parms:].reshape(x_shape)) / dx_f) ** 2) +266 return chisq +267 +268 if kwargs.get('expected_chisquare') is True: +269 W = np.diag(1 / np.asarray(np.concatenate((dy_f.ravel(), dx_f.ravel())))) +270 +271 if kwargs.get('covariance') is not None: +272 cov = kwargs.get('covariance') +273 else: +274 cov = covariance(np.concatenate((y, x.ravel()))) 275 -276 old_jac = jacobian(func)(out.beta, out.xplus) -277 fused_row1 = np.concatenate((old_jac, np.concatenate((number_of_x_parameters * [np.zeros(old_jac.shape)]), axis=0))) -278 fused_row2 = np.concatenate((jacobian(lambda x, y: func(y, x))(out.xplus, out.beta).reshape(x_f.shape[-1], x_f.shape[-1] * number_of_x_parameters), np.identity(number_of_x_parameters * old_jac.shape[0]))) -279 new_jac = np.concatenate((fused_row1, fused_row2), axis=1) -280 -281 A = W @ new_jac -282 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T -283 expected_chisquare = np.trace((np.identity(P_phi.shape[0]) - P_phi) @ W @ cov @ W) -284 if expected_chisquare <= 0.0: -285 warnings.warn("Negative expected_chisquare.", RuntimeWarning) -286 expected_chisquare = np.abs(expected_chisquare) -287 output.chisquare_by_expected_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) / expected_chisquare -288 if not silent: -289 print('chisquare/expected_chisquare:', -290 output.chisquare_by_expected_chisquare) -291 -292 fitp = out.beta -293 try: -294 hess = hessian(odr_chisquare)(np.concatenate((fitp, out.xplus.ravel()))) -295 except TypeError: -296 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None -297 -298 def odr_chisquare_compact_x(d): -299 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) -300 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((d[n_parms + m:].reshape(x_shape) - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) -301 return chisq -302 -303 jac_jac_x = hessian(odr_chisquare_compact_x)(np.concatenate((fitp, out.xplus.ravel(), x_f.ravel()))) +276 number_of_x_parameters = int(m / x_f.shape[-1]) +277 +278 old_jac = jacobian(func)(out.beta, out.xplus) +279 fused_row1 = np.concatenate((old_jac, np.concatenate((number_of_x_parameters * [np.zeros(old_jac.shape)]), axis=0))) +280 fused_row2 = np.concatenate((jacobian(lambda x, y: func(y, x))(out.xplus, out.beta).reshape(x_f.shape[-1], x_f.shape[-1] * number_of_x_parameters), np.identity(number_of_x_parameters * old_jac.shape[0]))) +281 new_jac = np.concatenate((fused_row1, fused_row2), axis=1) +282 +283 A = W @ new_jac +284 P_phi = A @ np.linalg.pinv(A.T @ A) @ A.T +285 expected_chisquare = np.trace((np.identity(P_phi.shape[0]) - P_phi) @ W @ cov @ W) +286 if expected_chisquare <= 0.0: +287 warnings.warn("Negative expected_chisquare.", RuntimeWarning) +288 expected_chisquare = np.abs(expected_chisquare) +289 output.chisquare_by_expected_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) / expected_chisquare +290 if not silent: +291 print('chisquare/expected_chisquare:', +292 output.chisquare_by_expected_chisquare) +293 +294 fitp = out.beta +295 try: +296 hess = hessian(odr_chisquare)(np.concatenate((fitp, out.xplus.ravel()))) +297 except TypeError: +298 raise Exception("It is required to use autograd.numpy instead of numpy within fit functions, see the documentation for details.") from None +299 +300 def odr_chisquare_compact_x(d): +301 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) +302 chisq = anp.sum(((y_f - model) / dy_f) ** 2) + anp.sum(((d[n_parms + m:].reshape(x_shape) - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) +303 return chisq 304 -305 # Compute hess^{-1} @ jac_jac_x[:n_parms + m, n_parms + m:] using LAPACK dgesv -306 try: -307 deriv_x = -scipy.linalg.solve(hess, jac_jac_x[:n_parms + m, n_parms + m:]) -308 except np.linalg.LinAlgError: -309 raise Exception("Cannot invert hessian matrix.") -310 -311 def odr_chisquare_compact_y(d): -312 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) -313 chisq = anp.sum(((d[n_parms + m:] - model) / dy_f) ** 2) + anp.sum(((x_f - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) -314 return chisq -315 -316 jac_jac_y = hessian(odr_chisquare_compact_y)(np.concatenate((fitp, out.xplus.ravel(), y_f))) +305 jac_jac_x = hessian(odr_chisquare_compact_x)(np.concatenate((fitp, out.xplus.ravel(), x_f.ravel()))) +306 +307 # Compute hess^{-1} @ jac_jac_x[:n_parms + m, n_parms + m:] using LAPACK dgesv +308 try: +309 deriv_x = -scipy.linalg.solve(hess, jac_jac_x[:n_parms + m, n_parms + m:]) +310 except np.linalg.LinAlgError: +311 raise Exception("Cannot invert hessian matrix.") +312 +313 def odr_chisquare_compact_y(d): +314 model = func(d[:n_parms], d[n_parms:n_parms + m].reshape(x_shape)) +315 chisq = anp.sum(((d[n_parms + m:] - model) / dy_f) ** 2) + anp.sum(((x_f - d[n_parms:n_parms + m].reshape(x_shape)) / dx_f) ** 2) +316 return chisq 317 -318 # Compute hess^{-1} @ jac_jac_y[:n_parms + m, n_parms + m:] using LAPACK dgesv -319 try: -320 deriv_y = -scipy.linalg.solve(hess, jac_jac_y[:n_parms + m, n_parms + m:]) -321 except np.linalg.LinAlgError: -322 raise Exception("Cannot invert hessian matrix.") -323 -324 result = [] -325 for i in range(n_parms): -326 result.append(derived_observable(lambda my_var, **kwargs: (my_var[0] + np.finfo(np.float64).eps) / (x.ravel()[0].value + np.finfo(np.float64).eps) * out.beta[i], list(x.ravel()) + list(y), man_grad=list(deriv_x[i]) + list(deriv_y[i]))) -327 -328 output.fit_parameters = result +318 jac_jac_y = hessian(odr_chisquare_compact_y)(np.concatenate((fitp, out.xplus.ravel(), y_f))) +319 +320 # Compute hess^{-1} @ jac_jac_y[:n_parms + m, n_parms + m:] using LAPACK dgesv +321 try: +322 deriv_y = -scipy.linalg.solve(hess, jac_jac_y[:n_parms + m, n_parms + m:]) +323 except np.linalg.LinAlgError: +324 raise Exception("Cannot invert hessian matrix.") +325 +326 result = [] +327 for i in range(n_parms): +328 result.append(derived_observable(lambda my_var, **kwargs: (my_var[0] + np.finfo(np.float64).eps) / (x.ravel()[0].value + np.finfo(np.float64).eps) * out.beta[i], list(x.ravel()) + list(y), man_grad=list(deriv_x[i]) + list(deriv_y[i]))) 329 -330 output.odr_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) -331 output.dof = x.shape[-1] - n_parms -332 output.p_value = 1 - scipy.stats.chi2.cdf(output.odr_chisquare, output.dof) -333 -334 return output +330 output.fit_parameters = result +331 +332 output.odr_chisquare = odr_chisquare(np.concatenate((out.beta, out.xplus.ravel()))) +333 output.dof = x.shape[-1] - n_parms +334 output.p_value = 1 - scipy.stats.chi2.cdf(output.odr_chisquare, output.dof) +335 +336 return output
660def fit_lin(x, y, **kwargs): -661 """Performs a linear fit to y = n + m * x and returns two Obs n, m. -662 -663 Parameters -664 ---------- -665 x : list -666 Can either be a list of floats in which case no xerror is assumed, or -667 a list of Obs, where the dvalues of the Obs are used as xerror for the fit. -668 y : list -669 List of Obs, the dvalues of the Obs are used as yerror for the fit. -670 """ -671 -672 def f(a, x): -673 y = a[0] + a[1] * x -674 return y -675 -676 if all(isinstance(n, Obs) for n in x): -677 out = total_least_squares(x, y, f, **kwargs) -678 return out.fit_parameters -679 elif all(isinstance(n, float) or isinstance(n, int) for n in x) or isinstance(x, np.ndarray): -680 out = least_squares(x, y, f, **kwargs) -681 return out.fit_parameters -682 else: -683 raise Exception('Unsupported types for x') +@@ -1509,30 +1538,30 @@ List of Obs, the dvalues of the Obs are used as yerror for the fit.662def fit_lin(x, y, **kwargs): +663 """Performs a linear fit to y = n + m * x and returns two Obs n, m. +664 +665 Parameters +666 ---------- +667 x : list +668 Can either be a list of floats in which case no xerror is assumed, or +669 a list of Obs, where the dvalues of the Obs are used as xerror for the fit. +670 y : list +671 List of Obs, the dvalues of the Obs are used as yerror for the fit. +672 """ +673 +674 def f(a, x): +675 y = a[0] + a[1] * x +676 return y +677 +678 if all(isinstance(n, Obs) for n in x): +679 out = total_least_squares(x, y, f, **kwargs) +680 return out.fit_parameters +681 elif all(isinstance(n, float) or isinstance(n, int) for n in x) or isinstance(x, np.ndarray): +682 out = least_squares(x, y, f, **kwargs) +683 return out.fit_parameters +684 else: +685 raise Exception('Unsupported types for x')
686def qqplot(x, o_y, func, p): -687 """Generates a quantile-quantile plot of the fit result which can be used to -688 check if the residuals of the fit are gaussian distributed. -689 """ -690 -691 residuals = [] -692 for i_x, i_y in zip(x, o_y): -693 residuals.append((i_y - func(p, i_x)) / i_y.dvalue) -694 residuals = sorted(residuals) -695 my_y = [o.value for o in residuals] -696 probplot = scipy.stats.probplot(my_y) -697 my_x = probplot[0][0] -698 plt.figure(figsize=(8, 8 / 1.618)) -699 plt.errorbar(my_x, my_y, fmt='o') -700 fit_start = my_x[0] -701 fit_stop = my_x[-1] -702 samples = np.arange(fit_start, fit_stop, 0.01) -703 plt.plot(samples, samples, 'k--', zorder=11, label='Standard normal distribution') -704 plt.plot(samples, probplot[1][0] * samples + probplot[1][1], zorder=10, label='Least squares fit, r=' + str(np.around(probplot[1][2], 3)), marker='', ls='-') -705 -706 plt.xlabel('Theoretical quantiles') -707 plt.ylabel('Ordered Values') -708 plt.legend() -709 plt.draw() +@@ -1553,34 +1582,34 @@ check if the residuals of the fit are gaussian distributed.688def qqplot(x, o_y, func, p): +689 """Generates a quantile-quantile plot of the fit result which can be used to +690 check if the residuals of the fit are gaussian distributed. +691 """ +692 +693 residuals = [] +694 for i_x, i_y in zip(x, o_y): +695 residuals.append((i_y - func(p, i_x)) / i_y.dvalue) +696 residuals = sorted(residuals) +697 my_y = [o.value for o in residuals] +698 probplot = scipy.stats.probplot(my_y) +699 my_x = probplot[0][0] +700 plt.figure(figsize=(8, 8 / 1.618)) +701 plt.errorbar(my_x, my_y, fmt='o') +702 fit_start = my_x[0] +703 fit_stop = my_x[-1] +704 samples = np.arange(fit_start, fit_stop, 0.01) +705 plt.plot(samples, samples, 'k--', zorder=11, label='Standard normal distribution') +706 plt.plot(samples, probplot[1][0] * samples + probplot[1][1], zorder=10, label='Least squares fit, r=' + str(np.around(probplot[1][2], 3)), marker='', ls='-') +707 +708 plt.xlabel('Theoretical quantiles') +709 plt.ylabel('Ordered Values') +710 plt.legend() +711 plt.draw()
712def residual_plot(x, y, func, fit_res): -713 """ Generates a plot which compares the fit to the data and displays the corresponding residuals""" -714 sorted_x = sorted(x) -715 xstart = sorted_x[0] - 0.5 * (sorted_x[1] - sorted_x[0]) -716 xstop = sorted_x[-1] + 0.5 * (sorted_x[-1] - sorted_x[-2]) -717 x_samples = np.arange(xstart, xstop + 0.01, 0.01) -718 -719 plt.figure(figsize=(8, 8 / 1.618)) -720 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) -721 ax0 = plt.subplot(gs[0]) -722 ax0.errorbar(x, [o.value for o in y], yerr=[o.dvalue for o in y], ls='none', fmt='o', capsize=3, markersize=5, label='Data') -723 ax0.plot(x_samples, func([o.value for o in fit_res], x_samples), label='Fit', zorder=10, ls='-', ms=0) -724 ax0.set_xticklabels([]) -725 ax0.set_xlim([xstart, xstop]) +@@ -1600,22 +1629,22 @@ check if the residuals of the fit are gaussian distributed.714def residual_plot(x, y, func, fit_res): +715 """ Generates a plot which compares the fit to the data and displays the corresponding residuals""" +716 sorted_x = sorted(x) +717 xstart = sorted_x[0] - 0.5 * (sorted_x[1] - sorted_x[0]) +718 xstop = sorted_x[-1] + 0.5 * (sorted_x[-1] - sorted_x[-2]) +719 x_samples = np.arange(xstart, xstop + 0.01, 0.01) +720 +721 plt.figure(figsize=(8, 8 / 1.618)) +722 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) +723 ax0 = plt.subplot(gs[0]) +724 ax0.errorbar(x, [o.value for o in y], yerr=[o.dvalue for o in y], ls='none', fmt='o', capsize=3, markersize=5, label='Data') +725 ax0.plot(x_samples, func([o.value for o in fit_res], x_samples), label='Fit', zorder=10, ls='-', ms=0) 726 ax0.set_xticklabels([]) -727 ax0.legend() -728 -729 residuals = (np.asarray([o.value for o in y]) - func([o.value for o in fit_res], x)) / np.asarray([o.dvalue for o in y]) -730 ax1 = plt.subplot(gs[1]) -731 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) -732 ax1.tick_params(direction='out') -733 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) -734 ax1.axhline(y=0.0, ls='--', color='k', marker=" ") -735 ax1.fill_between(x_samples, -1.0, 1.0, alpha=0.1, facecolor='k') -736 ax1.set_xlim([xstart, xstop]) -737 ax1.set_ylabel('Residuals') -738 plt.subplots_adjust(wspace=None, hspace=None) -739 plt.draw() +727 ax0.set_xlim([xstart, xstop]) +728 ax0.set_xticklabels([]) +729 ax0.legend() +730 +731 residuals = (np.asarray([o.value for o in y]) - func([o.value for o in fit_res], x)) / np.asarray([o.dvalue for o in y]) +732 ax1 = plt.subplot(gs[1]) +733 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) +734 ax1.tick_params(direction='out') +735 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) +736 ax1.axhline(y=0.0, ls='--', color='k', marker=" ") +737 ax1.fill_between(x_samples, -1.0, 1.0, alpha=0.1, facecolor='k') +738 ax1.set_xlim([xstart, xstop]) +739 ax1.set_ylabel('Residuals') +740 plt.subplots_adjust(wspace=None, hspace=None) +741 plt.draw()
742def error_band(x, func, beta): -743 """Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.""" -744 cov = covariance(beta) -745 if np.any(np.abs(cov - cov.T) > 1000 * np.finfo(np.float64).eps): -746 warnings.warn("Covariance matrix is not symmetric within floating point precision", RuntimeWarning) -747 -748 deriv = [] -749 for i, item in enumerate(x): -750 deriv.append(np.array(egrad(func)([o.value for o in beta], item))) -751 -752 err = [] -753 for i, item in enumerate(x): -754 err.append(np.sqrt(deriv[i] @ cov @ deriv[i])) -755 err = np.array(err) -756 -757 return err +@@ -1635,44 +1664,44 @@ check if the residuals of the fit are gaussian distributed.744def error_band(x, func, beta): +745 """Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.""" +746 cov = covariance(beta) +747 if np.any(np.abs(cov - cov.T) > 1000 * np.finfo(np.float64).eps): +748 warnings.warn("Covariance matrix is not symmetric within floating point precision", RuntimeWarning) +749 +750 deriv = [] +751 for i, item in enumerate(x): +752 deriv.append(np.array(egrad(func)([o.value for o in beta], item))) +753 +754 err = [] +755 for i, item in enumerate(x): +756 err.append(np.sqrt(deriv[i] @ cov @ deriv[i])) +757 err = np.array(err) +758 +759 return err
760def ks_test(objects=None): -761 """Performs a Kolmogorov–Smirnov test for the p-values of all fit object. -762 -763 Parameters -764 ---------- -765 objects : list -766 List of fit results to include in the analysis (optional). -767 """ -768 -769 if objects is None: -770 obs_list = [] -771 for obj in gc.get_objects(): -772 if isinstance(obj, Fit_result): -773 obs_list.append(obj) -774 else: -775 obs_list = objects -776 -777 p_values = [o.p_value for o in obs_list] +diff --git a/docs/search.js b/docs/search.js index 24bf5557..38f25af0 100644 --- a/docs/search.js +++ b/docs/search.js @@ -1,6 +1,6 @@ window.pdocSearch = (function(){ /** elasticlunr - http://weixsong.github.io * Copyright (C) 2017 Oliver Nightingale * Copyright (C) 2017 Wei Song * MIT Licensed */!function(){function e(e){if(null===e||"object"!=typeof e)return e;var t=e.constructor();for(var n in e)e.hasOwnProperty(n)&&(t[n]=e[n]);return t}var t=function(e){var n=new t.Index;return n.pipeline.add(t.trimmer,t.stopWordFilter,t.stemmer),e&&e.call(n,n),n};t.version="0.9.5",lunr=t,t.utils={},t.utils.warn=function(e){return function(t){e.console&&console.warn&&console.warn(t)}}(this),t.utils.toString=function(e){return void 0===e||null===e?"":e.toString()},t.EventEmitter=function(){this.events={}},t.EventEmitter.prototype.addListener=function(){var e=Array.prototype.slice.call(arguments),t=e.pop(),n=e;if("function"!=typeof t)throw new TypeError("last argument must be a function");n.forEach(function(e){this.hasHandler(e)||(this.events[e]=[]),this.events[e].push(t)},this)},t.EventEmitter.prototype.removeListener=function(e,t){if(this.hasHandler(e)){var n=this.events[e].indexOf(t);-1!==n&&(this.events[e].splice(n,1),0==this.events[e].length&&delete this.events[e])}},t.EventEmitter.prototype.emit=function(e){if(this.hasHandler(e)){var t=Array.prototype.slice.call(arguments,1);this.events[e].forEach(function(e){e.apply(void 0,t)},this)}},t.EventEmitter.prototype.hasHandler=function(e){return e in this.events},t.tokenizer=function(e){if(!arguments.length||null===e||void 0===e)return[];if(Array.isArray(e)){var n=e.filter(function(e){return null===e||void 0===e?!1:!0});n=n.map(function(e){return t.utils.toString(e).toLowerCase()});var i=[];return n.forEach(function(e){var n=e.split(t.tokenizer.seperator);i=i.concat(n)},this),i}return e.toString().trim().toLowerCase().split(t.tokenizer.seperator)},t.tokenizer.defaultSeperator=/[\s\-]+/,t.tokenizer.seperator=t.tokenizer.defaultSeperator,t.tokenizer.setSeperator=function(e){null!==e&&void 0!==e&&"object"==typeof e&&(t.tokenizer.seperator=e)},t.tokenizer.resetSeperator=function(){t.tokenizer.seperator=t.tokenizer.defaultSeperator},t.tokenizer.getSeperator=function(){return t.tokenizer.seperator},t.Pipeline=function(){this._queue=[]},t.Pipeline.registeredFunctions={},t.Pipeline.registerFunction=function(e,n){n in t.Pipeline.registeredFunctions&&t.utils.warn("Overwriting existing registered function: "+n),e.label=n,t.Pipeline.registeredFunctions[n]=e},t.Pipeline.getRegisteredFunction=function(e){return e in t.Pipeline.registeredFunctions!=!0?null:t.Pipeline.registeredFunctions[e]},t.Pipeline.warnIfFunctionNotRegistered=function(e){var n=e.label&&e.label in this.registeredFunctions;n||t.utils.warn("Function is not registered with pipeline. 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Xs -792 loc_max_diff = np.argmax(np.abs(diffs)) -793 loc = Xs[loc_max_diff] -794 plt.annotate('', xy=(loc, loc), xytext=(loc, loc + diffs[loc_max_diff]), arrowprops=dict(arrowstyle='<->', shrinkA=0, shrinkB=0)) -795 plt.draw() -796 -797 print(scipy.stats.kstest(p_values, 'uniform')) +779 p_values = [o.p_value for o in obs_list] +780 +781 bins = len(p_values) +782 x = np.arange(0, 1.001, 0.001) +783 plt.plot(x, x, 'k', zorder=1) +784 plt.xlim(0, 1) +785 plt.ylim(0, 1) +786 plt.xlabel('p-value') +787 plt.ylabel('Cumulative probability') +788 plt.title(str(bins) + ' p-values') +789 +790 n = np.arange(1, bins + 1) / np.float64(bins) +791 Xs = np.sort(p_values) +792 plt.step(Xs, n) +793 diffs = n - Xs +794 loc_max_diff = np.argmax(np.abs(diffs)) +795 loc = Xs[loc_max_diff] +796 plt.annotate('', xy=(loc, loc), xytext=(loc, loc + diffs[loc_max_diff]), arrowprops=dict(arrowstyle='<->', shrinkA=0, shrinkB=0)) +797 plt.draw() +798 +799 print(scipy.stats.kstest(p_values, 'uniform'))0&&t.push(e);for(var i in n)"docs"!==i&&"df"!==i&&this.expandToken(e+i,t,n[i]);return t},t.InvertedIndex.prototype.toJSON=function(){return{root:this.root}},t.Configuration=function(e,n){var e=e||"";if(void 0==n||null==n)throw new Error("fields should not be null");this.config={};var i;try{i=JSON.parse(e),this.buildUserConfig(i,n)}catch(o){t.utils.warn("user configuration parse failed, will use default configuration"),this.buildDefaultConfig(n)}},t.Configuration.prototype.buildDefaultConfig=function(e){this.reset(),e.forEach(function(e){this.config[e]={boost:1,bool:"OR",expand:!1}},this)},t.Configuration.prototype.buildUserConfig=function(e,n){var i="OR",o=!1;if(this.reset(),"bool"in e&&(i=e.bool||i),"expand"in e&&(o=e.expand||o),"fields"in e)for(var r in e.fields)if(n.indexOf(r)>-1){var s=e.fields[r],u=o;void 0!=s.expand&&(u=s.expand),this.config[r]={boost:s.boost||0===s.boost?s.boost:1,bool:s.bool||i,expand:u}}else t.utils.warn("field name in user configuration not found in index instance fields");else this.addAllFields2UserConfig(i,o,n)},t.Configuration.prototype.addAllFields2UserConfig=function(e,t,n){n.forEach(function(n){this.config[n]={boost:1,bool:e,expand:t}},this)},t.Configuration.prototype.get=function(){return this.config},t.Configuration.prototype.reset=function(){this.config={}},lunr.SortedSet=function(){this.length=0,this.elements=[]},lunr.SortedSet.load=function(e){var t=new this;return t.elements=e,t.length=e.length,t},lunr.SortedSet.prototype.add=function(){var e,t;for(e=0;e 1;){if(r===e)return o;e>r&&(t=o),r>e&&(n=o),i=n-t,o=t+Math.floor(i/2),r=this.elements[o]}return r===e?o:-1},lunr.SortedSet.prototype.locationFor=function(e){for(var t=0,n=this.elements.length,i=n-t,o=t+Math.floor(i/2),r=this.elements[o];i>1;)e>r&&(t=o),r>e&&(n=o),i=n-t,o=t+Math.floor(i/2),r=this.elements[o];return r>e?o:e>r?o+1:void 0},lunr.SortedSet.prototype.intersect=function(e){for(var t=new lunr.SortedSet,n=0,i=0,o=this.length,r=e.length,s=this.elements,u=e.elements;;){if(n>o-1||i>r-1)break;s[n]!==u[i]?s[n]u[i]&&i++:(t.add(s[n]),n++,i++)}return t},lunr.SortedSet.prototype.clone=function(){var e=new lunr.SortedSet;return e.elements=this.toArray(),e.length=e.elements.length,e},lunr.SortedSet.prototype.union=function(e){var t,n,i;this.length>=e.length?(t=this,n=e):(t=e,n=this),i=t.clone();for(var o=0,r=n.toArray();o What is pyerrors?\n\n \n\n
pyerrors
is a python package for error computation and propagation of Markov chain Monte Carlo data.\nIt is based on the gamma method arXiv:hep-lat/0306017. Some of its features are:\n
\n\n- automatic differentiation for exact linear error propagation as suggested in arXiv:1809.01289 (partly based on the autograd package).
\n- treatment of slow modes in the simulation as suggested in arXiv:1009.5228.
\n- coherent error propagation for data from different Markov chains.
\n- non-linear fits with x- and y-errors and exact linear error propagation based on automatic differentiation as introduced in arXiv:1809.01289.
\n- real and complex matrix operations and their error propagation based on automatic differentiation (Matrix inverse, Cholesky decomposition, calculation of eigenvalues and eigenvectors, singular value decomposition...).
\nMore detailed examples can found in the GitHub repository
\n\n.
If you use
\n\npyerrors
for research that leads to a publication please consider citing:\n
\n\n- Fabian Joswig, Simon Kuberski, Justus T. Kuhlmann, Jan Neuendorf, pyerrors: a python framework for error analysis of Monte Carlo data. [arXiv:2209.14371 [hep-lat]].
\n- Ulli Wolff, Monte Carlo errors with less errors. Comput.Phys.Commun. 156 (2004) 143-153, Comput.Phys.Commun. 176 (2007) 383 (erratum).
\n- Alberto Ramos, Automatic differentiation for error analysis of Monte Carlo data. Comput.Phys.Commun. 238 (2019) 19-35.
\nand
\n\n\n
\n\n- Stefan Schaefer, Rainer Sommer, Francesco Virotta, Critical slowing down and error analysis in lattice QCD simulations. Nucl.Phys.B 845 (2011) 93-119.
\nwhere applicable.
\n\nThere exist similar publicly available implementations of gamma method error analysis suites in Fortran, Julia and Python.
\n\nBasic example
\n\n\n\n\n\nimport numpy as np\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name']) # Initialize an Obs object\nmy_new_obs = 2 * np.log(my_obs) / my_obs ** 2 # Construct derived Obs object\nmy_new_obs.gamma_method() # Estimate the statistical error\nprint(my_new_obs) # Print the result to stdout\n> 0.31498(72)\n
The
\n\nObs
class\n\n
pyerrors
introduces a new datatype,Obs
, which simplifies error propagation and estimation for auto- and cross-correlated data.\nAnObs
object can be initialized with two arguments, the first is a list containing the samples for an observable from a Monte Carlo chain.\nThe samples can either be provided as python list or as numpy array.\nThe second argument is a list containing the names of the respective Monte Carlo chains as strings. These strings uniquely identify a Monte Carlo chain/ensemble.\n\n\n\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name'])\n
Error propagation
\n\nWhen performing mathematical operations on
\n\nObs
objects the correct error propagation is intrinsically taken care of using a first order Taylor expansion\n$$\\delta_f^i=\\sum_\\alpha \\bar{f}_\\alpha \\delta_\\alpha^i\\,,\\quad \\delta_\\alpha^i=a_\\alpha^i-\\bar{a}_\\alpha\\,,$$\nas introduced in arXiv:hep-lat/0306017.\nThe required derivatives $\\bar{f}_\\alpha$ are evaluated up to machine precision via automatic differentiation as suggested in arXiv:1809.01289.The
\n\nObs
class is designed such that mathematical numpy functions can be used onObs
just as for regular floats.\n\n\n\nimport numpy as np\nimport pyerrors as pe\n\nmy_obs1 = pe.Obs([samples1], ['ensemble_name'])\nmy_obs2 = pe.Obs([samples2], ['ensemble_name'])\n\nmy_sum = my_obs1 + my_obs2\n\nmy_m_eff = np.log(my_obs1 / my_obs2)\n\niamzero = my_m_eff - my_m_eff\n# Check that value and fluctuations are zero within machine precision\nprint(iamzero == 0.0)\n> True\n
Error estimation
\n\nThe error estimation within
\n\npyerrors
is based on the gamma method introduced in arXiv:hep-lat/0306017.\nAfter having arrived at the derived quantity of interest thegamma_method
can be called as detailed in the following example.\n\n\n\nmy_sum.gamma_method()\nprint(my_sum)\n> 1.70(57)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 5.72046658e-01 +/- 7.56746598e-02 (33.650%)\n> t_int 2.71422900e+00 +/- 6.40320983e-01 S = 2.00\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
We use the following definition of the integrated autocorrelation time established in Madras & Sokal 1988\n$$\\tau_\\mathrm{int}=\\frac{1}{2}+\\sum_{t=1}^{W}\\rho(t)\\geq \\frac{1}{2}\\,.$$\nThe window $W$ is determined via the automatic windowing procedure described in arXiv:hep-lat/0306017.\nThe standard value for the parameter $S$ of this automatic windowing procedure is $S=2$. Other values for $S$ can be passed to the
\n\ngamma_method
as parameter.\n\n\n\nmy_sum.gamma_method(S=3.0)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 6.30675201e-01 +/- 1.04585650e-01 (37.099%)\n> t_int 3.29909703e+00 +/- 9.77310102e-01 S = 3.00\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
The integrated autocorrelation time $\\tau_\\mathrm{int}$ and the autocorrelation function $\\rho(W)$ can be monitored via the methods
\n\npyerrors.obs.Obs.plot_tauint
andpyerrors.obs.Obs.plot_rho
.If the parameter $S$ is set to zero it is assumed that the dataset does not exhibit any autocorrelation and the window size is chosen to be zero.\nIn this case the error estimate is identical to the sample standard error.
\n\nExponential tails
\n\nSlow modes in the Monte Carlo history can be accounted for by attaching an exponential tail to the autocorrelation function $\\rho$ as suggested in arXiv:1009.5228. The longest autocorrelation time in the history, $\\tau_\\mathrm{exp}$, can be passed to the
\n\ngamma_method
as parameter. In this case the automatic windowing procedure is vacated and the parameter $S$ does not affect the error estimate.\n\n\n\nmy_sum.gamma_method(tau_exp=7.2)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 6.28097762e-01 +/- 5.79077524e-02 (36.947%)\n> t_int 3.27218667e+00 +/- 7.99583654e-01 tau_exp = 7.20, N_sigma = 1\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
For the full API see
\n\npyerrors.obs.Obs.gamma_method
.Multiple ensembles/replica
\n\nError propagation for multiple ensembles (Markov chains with different simulation parameters) is handled automatically. Ensembles are uniquely identified by their
\n\nname
.\n\n\n\nobs1 = pe.Obs([samples1], ['ensemble1'])\nobs2 = pe.Obs([samples2], ['ensemble2'])\n\nmy_sum = obs1 + obs2\nmy_sum.details()\n> Result 2.00697958e+00\n> 1500 samples in 2 ensembles:\n> \u00b7 Ensemble 'ensemble1' : 1000 configurations (from 1 to 1000)\n> \u00b7 Ensemble 'ensemble2' : 500 configurations (from 1 to 500)\n
\n\n
pyerrors
identifies multiple replica (independent Markov chains with identical simulation parameters) by the vertical bar|
in the name of the data set.\n\n\n\nobs1 = pe.Obs([samples1], ['ensemble1|r01'])\nobs2 = pe.Obs([samples2], ['ensemble1|r02'])\n\n> my_sum = obs1 + obs2\n> my_sum.details()\n> Result 2.00697958e+00\n> 1500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1'\n> \u00b7 Replicum 'r01' : 1000 configurations (from 1 to 1000)\n> \u00b7 Replicum 'r02' : 500 configurations (from 1 to 500)\n
Error estimation for multiple ensembles
\n\nIn order to keep track of different error analysis parameters for different ensembles one can make use of global dictionaries as detailed in the following example.
\n\n\n\n\n\npe.Obs.S_dict['ensemble1'] = 2.5\npe.Obs.tau_exp_dict['ensemble2'] = 8.0\npe.Obs.tau_exp_dict['ensemble3'] = 2.0\n
In case the
\n\ngamma_method
is called without any parameters it will use the values specified in the dictionaries for the respective ensembles.\nPassing arguments to thegamma_method
still dominates over the dictionaries.Irregular Monte Carlo chains
\n\n\n\n
Obs
objects defined on irregular Monte Carlo chains can be initialized with the parameteridl
.\n\n\n\n# Observable defined on configurations 20 to 519\nobs1 = pe.Obs([samples1], ['ensemble1'], idl=[range(20, 520)])\nobs1.details()\n> Result 9.98319881e-01\n> 500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 500 configurations (from 20 to 519)\n\n# Observable defined on every second configuration between 5 and 1003\nobs2 = pe.Obs([samples2], ['ensemble1'], idl=[range(5, 1005, 2)])\nobs2.details()\n> Result 9.99100712e-01\n> 500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 500 configurations (from 5 to 1003 in steps of 2)\n\n# Observable defined on configurations 2, 9, 28, 29 and 501\nobs3 = pe.Obs([samples3], ['ensemble1'], idl=[[2, 9, 28, 29, 501]])\nobs3.details()\n> Result 1.01718064e+00\n> 5 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 5 configurations (irregular range)\n
\n\n
Obs
objects defined on regular and irregular histories of the same ensemble can be combined with each other and the correct error propagation and estimation is automatically taken care of.Warning: Irregular Monte Carlo chains can result in odd patterns in the autocorrelation functions.\nMake sure to check the autocorrelation time with e.g.
\n\npyerrors.obs.Obs.plot_rho
orpyerrors.obs.Obs.plot_tauint
.For the full API see
\n\npyerrors.obs.Obs
.Correlators
\n\nWhen one is not interested in single observables but correlation functions,
\n\npyerrors
offers theCorr
class which simplifies the corresponding error propagation and provides the user with a set of standard methods. In order to initialize aCorr
objects one needs to arrange the data as a list ofObs
\n\n\n\nmy_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3])\nprint(my_corr)\n> x0/a Corr(x0/a)\n> ------------------\n> 0 0.7957(80)\n> 1 0.5156(51)\n> 2 0.3227(33)\n> 3 0.2041(21)\n
In case the correlation functions are not defined on the outermost timeslices, for example because of fixed boundary conditions, a padding can be introduced.
\n\n\n\n\n\nmy_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3], padding=[1, 1])\nprint(my_corr)\n> x0/a Corr(x0/a)\n> ------------------\n> 0\n> 1 0.7957(80)\n> 2 0.5156(51)\n> 3 0.3227(33)\n> 4 0.2041(21)\n> 5\n
The individual entries of a correlator can be accessed via slicing
\n\n\n\n\n\nprint(my_corr[3])\n> 0.3227(33)\n
Error propagation with the
\n\nCorr
class works very similar toObs
objects. Mathematical operations are overloaded andCorr
objects can be computed together with otherCorr
objects,Obs
objects or real numbers and integers.\n\n\n\nmy_new_corr = 0.3 * my_corr[2] * my_corr * my_corr + 12 / my_corr\n
\n\n
pyerrors
provides the user with a set of regularly used methods for the manipulation of correlator objects:\n
\n\n- \n
Corr.gamma_method
applies the gamma method to all entries of the correlator.- \n
Corr.m_eff
to construct effective masses. Various variants for periodic and fixed temporal boundary conditions are available.- \n
Corr.deriv
returns the first derivative of the correlator asCorr
. Different discretizations of the numerical derivative are available.- \n
Corr.second_deriv
returns the second derivative of the correlator asCorr
. Different discretizations of the numerical derivative are available.- \n
Corr.symmetric
symmetrizes parity even correlations functions, assuming periodic boundary conditions.- \n
Corr.anti_symmetric
anti-symmetrizes parity odd correlations functions, assuming periodic boundary conditions.- \n
Corr.T_symmetry
averages a correlator with its time symmetry partner, assuming fixed boundary conditions.- \n
Corr.plateau
extracts a plateau value from the correlator in a given range.- \n
Corr.roll
periodically shifts the correlator.- \n
Corr.reverse
reverses the time ordering of the correlator.- \n
Corr.correlate
constructs a disconnected correlation function from the correlator and anotherCorr
orObs
object.- \n
Corr.reweight
reweights the correlator.\n\n
pyerrors
can also handle matrices of correlation functions and extract energy states from these matrices via a generalized eigenvalue problem (seepyerrors.correlators.Corr.GEVP
).For the full API see
\n\npyerrors.correlators.Corr
.Complex valued observables
\n\n\n\n
pyerrors
can handle complex valued observables via the classpyerrors.obs.CObs
.\nCObs
are initialized with a real and an imaginary part which both can beObs
valued.\n\n\n\nmy_real_part = pe.Obs([samples1], ['ensemble1'])\nmy_imag_part = pe.Obs([samples2], ['ensemble1'])\n\nmy_cobs = pe.CObs(my_real_part, my_imag_part)\nmy_cobs.gamma_method()\nprint(my_cobs)\n> (0.9959(91)+0.659(28)j)\n
Elementary mathematical operations are overloaded and samples are properly propagated as for the
\n\nObs
class.\n\n\n\nmy_derived_cobs = (my_cobs + my_cobs.conjugate()) / np.abs(my_cobs)\nmy_derived_cobs.gamma_method()\nprint(my_derived_cobs)\n> (1.668(23)+0.0j)\n
The
\n\nCovobs
classIn many projects, auxiliary data that is not based on Monte Carlo chains enters. Examples are experimentally determined mesons masses which are used to set the scale or renormalization constants. These numbers come with an error that has to be propagated through the analysis. The
\n\nCovobs
class allows to define such quantities inpyerrors
. Furthermore, external input might consist of correlated quantities. An example are the parameters of an interpolation formula, which are defined via mean values and a covariance matrix between all parameters. The contribution of the interpolation formula to the error of a derived quantity therefore might depend on the complete covariance matrix.This concept is built into the definition of
\n\nCovobs
. Inpyerrors
, external input is defined by $M$ mean values, a $M\\times M$ covariance matrix, where $M=1$ is permissible, and a name that uniquely identifies the covariance matrix. Below, we define the pion mass, based on its mean value and error, 134.9768(5). Note, that the square of the error enterscov_Obs
, since the second argument of this function is the covariance matrix of theCovobs
.\n\n\n\nimport pyerrors.obs as pe\n\nmpi = pe.cov_Obs(134.9768, 0.0005**2, 'pi^0 mass')\nmpi.gamma_method()\nmpi.details()\n> Result 1.34976800e+02 +/- 5.00000000e-04 +/- 0.00000000e+00 (0.000%)\n> pi^0 mass 5.00000000e-04\n> 0 samples in 1 ensemble:\n> \u00b7 Covobs 'pi^0 mass'\n
The resulting object
\n\nmpi
is anObs
that contains aCovobs
. In the following, it may be handled as any otherObs
. The contribution of the covariance matrix to the error of anObs
is determined from the $M \\times M$ covariance matrix $\\Sigma$ and the gradient of theObs
with respect to the external quantities, which is the $1\\times M$ Jacobian matrix $J$, via\n$$s = \\sqrt{J^T \\Sigma J}\\,,$$\nwhere the Jacobian is computed for each derived quantity via automatic differentiation.Correlated auxiliary data is defined similarly to above, e.g., via
\n\n\n\n\n\nRAP = pe.cov_Obs([16.7457, -19.0475], [[3.49591, -6.07560], [-6.07560, 10.5834]], 'R_AP, 1906.03445, (5.3a)')\nprint(RAP)\n> [Obs[16.7(1.9)], Obs[-19.0(3.3)]]\n
where
\n\nRAP
now is a list of twoObs
that contains the two correlated parameters.Since the gradient of a derived observable with respect to an external covariance matrix is propagated through the entire analysis, the
\n\nCovobs
class allows to quote the derivative of a result with respect to the external quantities. If these derivatives are published together with the result, small shifts in the definition of external quantities, e.g., the definition of the physical point, can be performed a posteriori based on the published information. This may help to compare results of different groups. The gradient of anObs
o
with respect to a covariance matrix with the identifying stringk
may be accessed via\n\n\n\no.covobs[k].grad\n
Error propagation in iterative algorithms
\n\n\n\n
pyerrors
supports exact linear error propagation for iterative algorithms like various variants of non-linear least squares fits or root finding. The derivatives required for the error propagation are calculated as described in arXiv:1809.01289.Least squares fits
\n\nStandard non-linear least square fits with errors on the dependent but not the independent variables can be performed with
\n\npyerrors.fits.least_squares
. As default solver the Levenberg-Marquardt algorithm implemented in scipy is used.Fit functions have to be of the following form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[1] * anp.exp(-a[0] * x)\n
It is important that numerical functions refer to
\n\nautograd.numpy
instead ofnumpy
for the automatic differentiation in iterative algorithms to work properly.Fits can then be performed via
\n\n\n\n\n\nfit_result = pe.fits.least_squares(x, y, func)\nprint("\\n", fit_result)\n> Fit with 2 parameters\n> Method: Levenberg-Marquardt\n> `ftol` termination condition is satisfied.\n> chisquare/d.o.f.: 0.9593035785160936\n\n> Goodness of fit:\n> \u03c7\u00b2/d.o.f. = 0.959304\n> p-value = 0.5673\n> Fit parameters:\n> 0 0.0548(28)\n> 1 1.933(64)\n
where x is a
\n\nlist
ornumpy.array
offloats
and y is alist
ornumpy.array
ofObs
.Data stored in
\n\nCorr
objects can be fitted directly using theCorr.fit
method.\n\n\n\nmy_corr = pe.Corr(y)\nfit_result = my_corr.fit(func, fitrange=[12, 25])\n
this can simplify working with absolute fit ranges and takes care of gaps in the data automatically.
\n\nFor fit functions with multiple independent variables the fit function can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
\n\n
pyerrors
also supports correlated fits which can be triggered via the parametercorrelated_fit=True
.\nDetails about how the required covariance matrix is estimated can be found inpyerrors.obs.covariance
.Direct visualizations of the performed fits can be triggered via
\n\nresplot=True
orqqplot=True
. For all available options seepyerrors.fits.least_squares
.Total least squares fits
\n\n\n\n
pyerrors
can also fit data with errors on both the dependent and independent variables using the total least squares method also referred to orthogonal distance regression as implemented in scipy, seepyerrors.fits.least_squares
. The syntax is identical to the standard least squares case, the only difference being thatx
also has to be alist
ornumpy.array
ofObs
.For the full API see
\n\npyerrors.fits
for fits andpyerrors.roots
for finding roots of functions.Matrix operations
\n\n\n\n
pyerrors
provides wrappers forObs
- andCObs
-valued matrix operations based onnumpy.linalg
. The supported functions include:\n
\n\n- \n
inv
for the matrix inverse.- \n
cholseky
for the Cholesky decomposition.- \n
det
for the matrix determinant.- \n
eigh
for eigenvalues and eigenvectors of hermitean matrices.- \n
eig
for eigenvalues of general matrices.- \n
pinv
for the Moore-Penrose pseudoinverse.- \n
svd
for the singular-value-decomposition.For the full API see
\n\npyerrors.linalg
.Export data
\n\nThe preferred exported file format within
\n\npyerrors
is json.gz. Files written to this format are valid JSON files that have been compressed using gzip. The structure of the content is inspired by the dobs format of the ALPHA collaboration. The aim of the format is to facilitate the storage of data in a self-contained way such that, even years after the creation of the file, it is possible to extract all necessary information:\n
\n\n- What observables are stored? Possibly: How exactly are they defined.
\n- How does each single ensemble or external quantity contribute to the error of the observable?
\n- Who did write the file when and on which machine?
\nThis can be achieved by storing all information in one single file. The export routines of
\n\npyerrors
are written such that as much information as possible is written automatically as described in the following example\n\n\n\nmy_obs = pe.Obs([samples], ["test_ensemble"])\nmy_obs.tag = "My observable"\n\npe.input.json.dump_to_json(my_obs, "test_output_file", description="This file contains a test observable")\n# For a single observable one can equivalently use the class method dump\nmy_obs.dump("test_output_file", description="This file contains a test observable")\n\ncheck = pe.input.json.load_json("test_output_file")\n\nprint(my_obs == check)\n> True\n
The format also allows to directly write out the content of
\n\nCorr
objects or lists and arrays ofObs
objects by passing the desired data topyerrors.input.json.dump_to_json
.json.gz format specification
\n\nThe first entries of the file provide optional auxiliary information:
\n\n\n
\n\n- \n
program
is a string that indicates which program was used to write the file.- \n
version
is a string that specifies the version of the format.- \n
who
is a string that specifies the user name of the creator of the file.- \n
date
is a string and contains the creation date of the file.- \n
host
is a string and contains the hostname of the machine where the file has been written.- \n
description
contains information on the content of the file. This field is not filled automatically inpyerrors
. The user is advised to provide as detailed information as possible in this field. Examples are: Input files of measurements or simulations, LaTeX formulae or references to publications to specify how the observables have been computed, details on the analysis strategy, ... This field may be any valid JSON type. Strings, arrays or objects (equivalent to dicts in python) are well suited to provide information.The only necessary entry of the file is the field\n-
\n\nobsdata
, an array that contains the actual data.Each entry of the array belongs to a single structure of observables. Currently, these structures can be either of
\n\nObs
,list
,numpy.ndarray
,Corr
. AllObs
inside a structure (with dimension > 0) have to be defined on the same set of configurations. Different structures, that are represented by entries of the arrayobsdata
, are treated independently. Each entry of the arrayobsdata
has the following required entries:\n
\n\n- \n
type
is a string that specifies the type of the structure. This allows to parse the content to the correct form after reading the file. It is always possible to interpret the content as list of Obs.- \n
value
is an array that contains the mean values of the Obs inside the structure.\nThe following entries are optional:- \n
layout
is a string that specifies the layout of multi-dimensional structures. Examples are \"2, 2\" for a 2x2 dimensional matrix or \"64, 4, 4\" for a Corr with $T=64$ and 4x4 matrices on each time slices. \"1\" denotes a single Obs. Multi-dimensional structures are stored in row-major format (see below).- \n
tag
is any JSON type. It contains additional information concerning the structure. Thetag
of anObs
inpyerrors
is written here.- \n
reweighted
is a Bool that may be used to specify, whether theObs
in the structure have been reweighted.- \n
data
is an array that contains the data from MC chains. We will define it below.- \n
cdata
is an array that contains the data from external quantities with an error (Covobs
inpyerrors
). We will define it below.The array
\n\ndata
contains the data from MC chains. Each entry of the array corresponds to one ensemble and contains:\n
\n\n- \n
id
, a string that contains the name of the ensemble- \n
replica
, an array that contains an entry per replica of the ensemble.Each entry of
\n\nreplica
contains\nname
, a string that contains the name of the replica\ndeltas
, an array that contains the actual data.Each entry in
\n\ndeltas
corresponds to one configuration of the replica and has $1+N$ many entries. The first entry is an integer that specifies the configuration number that, together with ensemble and replica name, may be used to uniquely identify the configuration on which the data has been obtained. The following N entries specify the deltas, i.e., the deviation of the observable from the mean value on this configuration, of eachObs
inside the structure. Multi-dimensional structures are stored in a row-major format. For primary observables, such as correlation functions, $value + delta_i$ matches the primary data obtained on the configuration.The array
\n\ncdata
contains information about the contribution of auxiliary observables, represented byCovobs
inpyerrors
, to the total error of the observables. Each entry of the array belongs to one auxiliary covariance matrix and contains:\n
\n\n- \n
id
, a string that identifies the covariance matrix- \n
layout
, a string that defines the dimensions of the $M\\times M$ covariance matrix (has to be \"M, M\" or \"1\").- \n
cov
, an array that contains the $M\\times M$ many entries of the covariance matrix, stored in row-major format.- \n
grad
, an array that contains N entries, one for eachObs
inside the structure. Each entry itself is an array, that contains the M gradients of the Nth observable with respect to the quantity that corresponds to the Mth diagonal entry of the covariance matrix.A JSON schema that may be used to verify the correctness of a file with respect to the format definition is stored in ./examples/json_schema.json. The schema is a self-descriptive format definition and contains an exemplary file.
\n\nJulia I/O routines for the json.gz format, compatible with ADerrors.jl, can be found here.
\n"}, "pyerrors.correlators": {"fullname": "pyerrors.correlators", "modulename": "pyerrors.correlators", "kind": "module", "doc": "\n"}, "pyerrors.correlators.Corr": {"fullname": "pyerrors.correlators.Corr", "modulename": "pyerrors.correlators", "qualname": "Corr", "kind": "class", "doc": "The class for a correlator (time dependent sequence of pe.Obs).
\n\nEverything, this class does, can be achieved using lists or arrays of Obs.\nBut it is simply more convenient to have a dedicated object for correlators.\nOne often wants to add or multiply correlators of the same length at every timeslice and it is inconvenient\nto iterate over all timeslices for every operation. This is especially true, when dealing with matrices.
\n\nThe correlator can have two types of content: An Obs at every timeslice OR a GEVP\nmatrix at every timeslice. Other dependency (eg. spatial) are not supported.
\n"}, "pyerrors.correlators.Corr.__init__": {"fullname": "pyerrors.correlators.Corr.__init__", "modulename": "pyerrors.correlators", "qualname": "Corr.__init__", "kind": "function", "doc": "Initialize a Corr object.
\n\nParameters
\n\n\n
\n", "signature": "(data_input, padding=[0, 0], prange=None)"}, "pyerrors.correlators.Corr.gamma_method": {"fullname": "pyerrors.correlators.Corr.gamma_method", "modulename": "pyerrors.correlators", "qualname": "Corr.gamma_method", "kind": "function", "doc": "- data_input (list or array):\nlist of Obs or list of arrays of Obs or array of Corrs
\n- padding (list, optional):\nList with two entries where the first labels the padding\nat the front of the correlator and the second the padding\nat the back.
\n- prange (list, optional):\nList containing the first and last timeslice of the plateau\nregion indentified for this correlator.
\nApply the gamma method to the content of the Corr.
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.projected": {"fullname": "pyerrors.correlators.Corr.projected", "modulename": "pyerrors.correlators", "qualname": "Corr.projected", "kind": "function", "doc": "We need to project the Correlator with a Vector to get a single value at each timeslice.
\n\nThe method can use one or two vectors.\nIf two are specified it returns v1@G@v2 (the order might be very important.)\nBy default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to
\n", "signature": "(self, vector_l=None, vector_r=None, normalize=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.item": {"fullname": "pyerrors.correlators.Corr.item", "modulename": "pyerrors.correlators", "qualname": "Corr.item", "kind": "function", "doc": "Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice.
\n\nParameters
\n\n\n
\n", "signature": "(self, i, j):", "funcdef": "def"}, "pyerrors.correlators.Corr.plottable": {"fullname": "pyerrors.correlators.Corr.plottable", "modulename": "pyerrors.correlators", "qualname": "Corr.plottable", "kind": "function", "doc": "- i (int):\nFirst index to be picked.
\n- j (int):\nSecond index to be picked.
\nOutputs the correlator in a plotable format.
\n\nOutputs three lists containing the timeslice index, the value on each\ntimeslice and the error on each timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.symmetric": {"fullname": "pyerrors.correlators.Corr.symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.symmetric", "kind": "function", "doc": "Symmetrize the correlator around x0=0.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.anti_symmetric": {"fullname": "pyerrors.correlators.Corr.anti_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.anti_symmetric", "kind": "function", "doc": "Anti-symmetrize the correlator around x0=0.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.is_matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.is_matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.is_matrix_symmetric", "kind": "function", "doc": "Checks whether a correlator matrices is symmetric on every timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.matrix_symmetric", "kind": "function", "doc": "Symmetrizes the correlator matrices on every timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.GEVP": {"fullname": "pyerrors.correlators.Corr.GEVP", "modulename": "pyerrors.correlators", "qualname": "Corr.GEVP", "kind": "function", "doc": "Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors.
\n\nThe eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the\nlargest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing
\n\n\n\n\n\nC.GEVP(t0=2)[0] # Ground state vector(s)\nC.GEVP(t0=2)[:3] # Vectors for the lowest three states\n
Parameters
\n\n\n
\n\n- t0 (int):\nThe time t0 for the right hand side of the GEVP according to $G(t)v_i=\\lambda_i G(t_0)v_i$
\n- ts (int):\nfixed time $G(t_s)v_i=\\lambda_i G(t_0)v_i$ if sort=None.\nIf sort=\"Eigenvector\" it gives a reference point for the sorting method.
\n- sort (string):\nIf this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned.\n
\n\n
- \"Eigenvalue\": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice.
\n- \"Eigenvector\": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state.\nThe reference state is identified by its eigenvalue at $t=t_s$.
\nOther Parameters
\n\n\n
\n", "signature": "(self, t0, ts=None, sort='Eigenvalue', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.Eigenvalue": {"fullname": "pyerrors.correlators.Corr.Eigenvalue", "modulename": "pyerrors.correlators", "qualname": "Corr.Eigenvalue", "kind": "function", "doc": "- state (int):\nReturns only the vector(s) for a specified state. The lowest state is zero.
\nDetermines the eigenvalue of the GEVP by solving and projecting the correlator
\n\nParameters
\n\n\n
\n", "signature": "(self, t0, ts=None, state=0, sort='Eigenvalue'):", "funcdef": "def"}, "pyerrors.correlators.Corr.Hankel": {"fullname": "pyerrors.correlators.Corr.Hankel", "modulename": "pyerrors.correlators", "qualname": "Corr.Hankel", "kind": "function", "doc": "- state (int):\nThe state one is interested in ordered by energy. The lowest state is zero.
\n- All other parameters are identical to the ones of Corr.GEVP.
\nConstructs an NxN Hankel matrix
\n\nC(t) c(t+1) ... c(t+n-1)\nC(t+1) c(t+2) ... c(t+n)\n.................\nC(t+(n-1)) c(t+n) ... c(t+2(n-1))
\n\nParameters
\n\n\n
\n", "signature": "(self, N, periodic=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.roll": {"fullname": "pyerrors.correlators.Corr.roll", "modulename": "pyerrors.correlators", "qualname": "Corr.roll", "kind": "function", "doc": "- N (int):\nDimension of the Hankel matrix
\n- periodic (bool, optional):\ndetermines whether the matrix is extended periodically
\nPeriodically shift the correlator by dt timeslices
\n\nParameters
\n\n\n
\n", "signature": "(self, dt):", "funcdef": "def"}, "pyerrors.correlators.Corr.reverse": {"fullname": "pyerrors.correlators.Corr.reverse", "modulename": "pyerrors.correlators", "qualname": "Corr.reverse", "kind": "function", "doc": "- dt (int):\nnumber of timeslices
\nReverse the time ordering of the Corr
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.thin": {"fullname": "pyerrors.correlators.Corr.thin", "modulename": "pyerrors.correlators", "qualname": "Corr.thin", "kind": "function", "doc": "Thin out a correlator to suppress correlations
\n\nParameters
\n\n\n
\n", "signature": "(self, spacing=2, offset=0):", "funcdef": "def"}, "pyerrors.correlators.Corr.correlate": {"fullname": "pyerrors.correlators.Corr.correlate", "modulename": "pyerrors.correlators", "qualname": "Corr.correlate", "kind": "function", "doc": "- spacing (int):\nKeep only every 'spacing'th entry of the correlator
\n- offset (int):\nOffset the equal spacing
\nCorrelate the correlator with another correlator or Obs
\n\nParameters
\n\n\n
\n", "signature": "(self, partner):", "funcdef": "def"}, "pyerrors.correlators.Corr.reweight": {"fullname": "pyerrors.correlators.Corr.reweight", "modulename": "pyerrors.correlators", "qualname": "Corr.reweight", "kind": "function", "doc": "- partner (Obs or Corr):\npartner to correlate the correlator with.\nCan either be an Obs which is correlated with all entries of the\ncorrelator or a Corr of same length.
\nReweight the correlator.
\n\nParameters
\n\n\n
\n", "signature": "(self, weight, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.T_symmetry": {"fullname": "pyerrors.correlators.Corr.T_symmetry", "modulename": "pyerrors.correlators", "qualname": "Corr.T_symmetry", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl.
\nReturn the time symmetry average of the correlator and its partner
\n\nParameters
\n\n\n
\n", "signature": "(self, partner, parity=1):", "funcdef": "def"}, "pyerrors.correlators.Corr.deriv": {"fullname": "pyerrors.correlators.Corr.deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.deriv", "kind": "function", "doc": "- partner (Corr):\nTime symmetry partner of the Corr
\n- partity (int):\nParity quantum number of the correlator, can be +1 or -1
\nReturn the first derivative of the correlator with respect to x0.
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.second_deriv": {"fullname": "pyerrors.correlators.Corr.second_deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.second_deriv", "kind": "function", "doc": "- variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, forward, backward, improved, log, default: symmetric
\nReturn the second derivative of the correlator with respect to x0.
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.m_eff": {"fullname": "pyerrors.correlators.Corr.m_eff", "modulename": "pyerrors.correlators", "qualname": "Corr.m_eff", "kind": "function", "doc": "- variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, improved, log, default: symmetric
\nReturns the effective mass of the correlator as correlator object
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='log', guess=1.0):", "funcdef": "def"}, "pyerrors.correlators.Corr.fit": {"fullname": "pyerrors.correlators.Corr.fit", "modulename": "pyerrors.correlators", "qualname": "Corr.fit", "kind": "function", "doc": "- variant (str):\nlog : uses the standard effective mass log(C(t) / C(t+1))\ncosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m.\nsinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m.\nSee, e.g., arXiv:1205.5380\narccosh : Uses the explicit form of the symmetrized correlator (not recommended)\nlogsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2
\n- guess (float):\nguess for the root finder, only relevant for the root variant
\nFits function to the data
\n\nParameters
\n\n\n
\n", "signature": "(self, function, fitrange=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.plateau": {"fullname": "pyerrors.correlators.Corr.plateau", "modulename": "pyerrors.correlators", "qualname": "Corr.plateau", "kind": "function", "doc": "- function (obj):\nfunction to fit to the data. See fits.least_squares for details.
\n- fitrange (list):\nTwo element list containing the timeslices on which the fit is supposed to start and stop.\nCaution: This range is inclusive as opposed to standard python indexing.\n
\nfitrange=[4, 6]
corresponds to the three entries 4, 5 and 6.\nIf not specified, self.prange or all timeslices are used.- silent (bool):\nDecides whether output is printed to the standard output.
\nExtract a plateau value from a Corr object
\n\nParameters
\n\n\n
\n", "signature": "(self, plateau_range=None, method='fit', auto_gamma=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.set_prange": {"fullname": "pyerrors.correlators.Corr.set_prange", "modulename": "pyerrors.correlators", "qualname": "Corr.set_prange", "kind": "function", "doc": "- plateau_range (list):\nlist with two entries, indicating the first and the last timeslice\nof the plateau region.
\n- method (str):\nmethod to extract the plateau.\n 'fit' fits a constant to the plateau region\n 'avg', 'average' or 'mean' just average over the given timeslices.
\n- auto_gamma (bool):\napply gamma_method with default parameters to the Corr. Defaults to None
\nSets the attribute prange of the Corr object.
\n", "signature": "(self, prange):", "funcdef": "def"}, "pyerrors.correlators.Corr.show": {"fullname": "pyerrors.correlators.Corr.show", "modulename": "pyerrors.correlators", "qualname": "Corr.show", "kind": "function", "doc": "Plots the correlator using the tag of the correlator as label if available.
\n\nParameters
\n\n\n
\n", "signature": "(\tself,\tx_range=None,\tcomp=None,\ty_range=None,\tlogscale=False,\tplateau=None,\tfit_res=None,\tylabel=None,\tsave=None,\tauto_gamma=False,\thide_sigma=None,\treferences=None,\ttitle=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.spaghetti_plot": {"fullname": "pyerrors.correlators.Corr.spaghetti_plot", "modulename": "pyerrors.correlators", "qualname": "Corr.spaghetti_plot", "kind": "function", "doc": "- x_range (list):\nlist of two values, determining the range of the x-axis e.g. [4, 8].
\n- comp (Corr or list of Corr):\nCorrelator or list of correlators which are plotted for comparison.\nThe tags of these correlators are used as labels if available.
\n- logscale (bool):\nSets y-axis to logscale.
\n- plateau (Obs):\nPlateau value to be visualized in the figure.
\n- fit_res (Fit_result):\nFit_result object to be visualized.
\n- ylabel (str):\nLabel for the y-axis.
\n- save (str):\npath to file in which the figure should be saved.
\n- auto_gamma (bool):\nApply the gamma method with standard parameters to all correlators and plateau values before plotting.
\n- hide_sigma (float):\nHides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors.
\n- references (list):\nList of floating point values that are displayed as horizontal lines for reference.
\n- title (string):\nOptional title of the figure.
\nProduces a spaghetti plot of the correlator suited to monitor exceptional configurations.
\n\nParameters
\n\n\n
\n", "signature": "(self, logscale=True):", "funcdef": "def"}, "pyerrors.correlators.Corr.dump": {"fullname": "pyerrors.correlators.Corr.dump", "modulename": "pyerrors.correlators", "qualname": "Corr.dump", "kind": "function", "doc": "- logscale (bool):\nDetermines whether the scale of the y-axis is logarithmic or standard.
\nDumps the Corr into a file of chosen type
\n\nParameters
\n\n\n
\n", "signature": "(self, filename, datatype='json.gz', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.print": {"fullname": "pyerrors.correlators.Corr.print", "modulename": "pyerrors.correlators", "qualname": "Corr.print", "kind": "function", "doc": "\n", "signature": "(self, print_range=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.sqrt": {"fullname": "pyerrors.correlators.Corr.sqrt", "modulename": "pyerrors.correlators", "qualname": "Corr.sqrt", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.log": {"fullname": "pyerrors.correlators.Corr.log", "modulename": "pyerrors.correlators", "qualname": "Corr.log", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.exp": {"fullname": "pyerrors.correlators.Corr.exp", "modulename": "pyerrors.correlators", "qualname": "Corr.exp", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sin": {"fullname": "pyerrors.correlators.Corr.sin", "modulename": "pyerrors.correlators", "qualname": "Corr.sin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cos": {"fullname": "pyerrors.correlators.Corr.cos", "modulename": "pyerrors.correlators", "qualname": "Corr.cos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tan": {"fullname": "pyerrors.correlators.Corr.tan", "modulename": "pyerrors.correlators", "qualname": "Corr.tan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sinh": {"fullname": "pyerrors.correlators.Corr.sinh", "modulename": "pyerrors.correlators", "qualname": "Corr.sinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cosh": {"fullname": "pyerrors.correlators.Corr.cosh", "modulename": "pyerrors.correlators", "qualname": "Corr.cosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tanh": {"fullname": "pyerrors.correlators.Corr.tanh", "modulename": "pyerrors.correlators", "qualname": "Corr.tanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsin": {"fullname": "pyerrors.correlators.Corr.arcsin", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccos": {"fullname": "pyerrors.correlators.Corr.arccos", "modulename": "pyerrors.correlators", "qualname": "Corr.arccos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctan": {"fullname": "pyerrors.correlators.Corr.arctan", "modulename": "pyerrors.correlators", "qualname": "Corr.arctan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsinh": {"fullname": "pyerrors.correlators.Corr.arcsinh", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccosh": {"fullname": "pyerrors.correlators.Corr.arccosh", "modulename": "pyerrors.correlators", "qualname": "Corr.arccosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctanh": {"fullname": "pyerrors.correlators.Corr.arctanh", "modulename": "pyerrors.correlators", "qualname": "Corr.arctanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.prune": {"fullname": "pyerrors.correlators.Corr.prune", "modulename": "pyerrors.correlators", "qualname": "Corr.prune", "kind": "function", "doc": "- filename (str):\nName of the file to be saved.
\n- datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
\n- path (str):\nspecifies a custom path for the file (default '.')
\nProject large correlation matrix to lowest states
\n\nThis method can be used to reduce the size of an (N x N) correlation matrix\nto (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise\nis still small.
\n\nParameters
\n\n\n
\n\n- Ntrunc (int):\nRank of the target matrix.
\n- tproj (int):\nTime where the eigenvectors are evaluated, corresponds to ts in the GEVP method.\nThe default value is 3.
\n- t0proj (int):\nTime where the correlation matrix is inverted. Choosing t0proj=1 is strongly\ndiscouraged for O(a) improved theories, since the correctness of the procedure\ncannot be granted in this case. The default value is 2.
\n- basematrix (Corr):\nCorrelation matrix that is used to determine the eigenvectors of the\nlowest states based on a GEVP. basematrix is taken to be the Corr itself if\nis is not specified.
\nNotes
\n\nWe have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving\nthe GEVP $$C(t) v_n(t, t_0) = \\lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \\equiv t_\\mathrm{proj}$\nand $t_0 \\equiv t_{0, \\mathrm{proj}}$. The target matrix is projected onto the subspace of the\nresulting eigenvectors $v_n, n=1,\\dots,N_\\mathrm{trunc}$ via\n$$G^\\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large\ncorrelation matrix and to remove some noise that is added by irrelevant operators.\nThis may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated\nbound $t_0 \\leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$.
\n", "signature": "(self, Ntrunc, tproj=3, t0proj=2, basematrix=None):", "funcdef": "def"}, "pyerrors.covobs": {"fullname": "pyerrors.covobs", "modulename": "pyerrors.covobs", "kind": "module", "doc": "\n"}, "pyerrors.covobs.Covobs": {"fullname": "pyerrors.covobs.Covobs", "modulename": "pyerrors.covobs", "qualname": "Covobs", "kind": "class", "doc": "\n"}, "pyerrors.covobs.Covobs.__init__": {"fullname": "pyerrors.covobs.Covobs.__init__", "modulename": "pyerrors.covobs", "qualname": "Covobs.__init__", "kind": "function", "doc": "Initialize Covobs object.
\n\nParameters
\n\n\n
\n", "signature": "(mean, cov, name, pos=None, grad=None)"}, "pyerrors.covobs.Covobs.errsq": {"fullname": "pyerrors.covobs.Covobs.errsq", "modulename": "pyerrors.covobs", "qualname": "Covobs.errsq", "kind": "function", "doc": "- mean (float):\nMean value of the new Obs
\n- cov (list or array):\n2d Covariance matrix or 1d diagonal entries
\n- name (str):\nidentifier for the covariance matrix
\n- pos (int):\nPosition of the variance belonging to mean in cov.\nIs taken to be 1 if cov is 0-dimensional
\n- grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
\nReturn the variance (= square of the error) of the Covobs
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.dirac": {"fullname": "pyerrors.dirac", "modulename": "pyerrors.dirac", "kind": "module", "doc": "\n"}, "pyerrors.dirac.epsilon_tensor": {"fullname": "pyerrors.dirac.epsilon_tensor", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor", "kind": "function", "doc": "Rank-3 epsilon tensor
\n\nBased on https://codegolf.stackexchange.com/a/160375
\n", "signature": "(i, j, k):", "funcdef": "def"}, "pyerrors.dirac.epsilon_tensor_rank4": {"fullname": "pyerrors.dirac.epsilon_tensor_rank4", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor_rank4", "kind": "function", "doc": "Rank-4 epsilon tensor
\n\nExtension of https://codegolf.stackexchange.com/a/160375
\n", "signature": "(i, j, k, o):", "funcdef": "def"}, "pyerrors.dirac.Grid_gamma": {"fullname": "pyerrors.dirac.Grid_gamma", "modulename": "pyerrors.dirac", "qualname": "Grid_gamma", "kind": "function", "doc": "Returns gamma matrix in Grid labeling.
\n", "signature": "(gamma_tag):", "funcdef": "def"}, "pyerrors.fits": {"fullname": "pyerrors.fits", "modulename": "pyerrors.fits", "kind": "module", "doc": "\n"}, "pyerrors.fits.Fit_result": {"fullname": "pyerrors.fits.Fit_result", "modulename": "pyerrors.fits", "qualname": "Fit_result", "kind": "class", "doc": "Represents fit results.
\n\nAttributes
\n\n\n
\n", "bases": "collections.abc.Sequence"}, "pyerrors.fits.Fit_result.__init__": {"fullname": "pyerrors.fits.Fit_result.__init__", "modulename": "pyerrors.fits", "qualname": "Fit_result.__init__", "kind": "function", "doc": "\n", "signature": "()"}, "pyerrors.fits.Fit_result.gamma_method": {"fullname": "pyerrors.fits.Fit_result.gamma_method", "modulename": "pyerrors.fits", "qualname": "Fit_result.gamma_method", "kind": "function", "doc": "- fit_parameters (list):\nresults for the individual fit parameters,\nalso accessible via indices.
\n- chisquare_by_dof (float):\nreduced chisquare.
\n- p_value (float):\np-value of the fit
\n- t2_p_value (float):\nHotelling t-squared p-value for correlated fits.
\nApply the gamma method to all fit parameters
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.least_squares": {"fullname": "pyerrors.fits.least_squares", "modulename": "pyerrors.fits", "qualname": "least_squares", "kind": "function", "doc": "Performs a non-linear fit to y = func(x).
\n\nParameters
\n\n\n
\n", "signature": "(x, y, func, priors=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.total_least_squares": {"fullname": "pyerrors.fits.total_least_squares", "modulename": "pyerrors.fits", "qualname": "total_least_squares", "kind": "function", "doc": "- x (list):\nlist of floats.
\n- y (list):\nlist of Obs.
\n- \n
func (object):\nfit function, has to be of the form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
For multiple x values func can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.
- priors (list, optional):\npriors has to be a list with an entry for every parameter in the fit. The entries can either be\nObs (e.g. results from a previous fit) or strings containing a value and an error formatted like\n0.548(23), 500(40) or 0.5(0.4)
\n- silent (bool, optional):\nIf true all output to the console is omitted (default False).
\n- initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for\nnon-linear fits with many parameters. In case of correlated fits the guess is used to perform\nan uncorrelated fit which then serves as guess for the correlated fit.
\n- method (str, optional):\ncan be used to choose an alternative method for the minimization of chisquare.\nThe possible methods are the ones which can be used for scipy.optimize.minimize and\nmigrad of iminuit. If no method is specified, Levenberg-Marquard is used.\nReliable alternatives are migrad, Powell and Nelder-Mead.
\n- correlated_fit (bool):\nIf True, use the full inverse covariance matrix in the definition of the chisquare cost function.\nFor details about how the covariance matrix is estimated see
\npyerrors.obs.covariance
.\nIn practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix).\nThis procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning).\nAt the moment this option only works forprior==None
and when nomethod
is given.- expected_chisquare (bool):\nIf True estimates the expected chisquare which is\ncorrected by effects caused by correlated input data (default False).
\n- resplot (bool):\nIf True, a plot which displays fit, data and residuals is generated (default False).
\n- qqplot (bool):\nIf True, a quantile-quantile plot of the fit result is generated (default False).
\n- num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
\nPerforms a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters.
\n\nParameters
\n\n\n
\n\n- x (list):\nlist of Obs, or a tuple of lists of Obs
\n- y (list):\nlist of Obs. The dvalues of the Obs are used as x- and yerror for the fit.
\n- \n
func (object):\nfunc has to be of the form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
For multiple x values func can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.
- silent (bool, optional):\nIf true all output to the console is omitted (default False).
\n- initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for non-linear\nfits with many parameters.
\n- expected_chisquare (bool):\nIf true prints the expected chisquare which is\ncorrected by effects caused by correlated input data.\nThis can take a while as the full correlation matrix\nhas to be calculated (default False).
\n- num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
\nNotes
\n\nBased on the orthogonal distance regression module of scipy
\n", "signature": "(x, y, func, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.fit_lin": {"fullname": "pyerrors.fits.fit_lin", "modulename": "pyerrors.fits", "qualname": "fit_lin", "kind": "function", "doc": "Performs a linear fit to y = n + m * x and returns two Obs n, m.
\n\nParameters
\n\n\n
\n", "signature": "(x, y, **kwargs):", "funcdef": "def"}, "pyerrors.fits.qqplot": {"fullname": "pyerrors.fits.qqplot", "modulename": "pyerrors.fits", "qualname": "qqplot", "kind": "function", "doc": "- x (list):\nCan either be a list of floats in which case no xerror is assumed, or\na list of Obs, where the dvalues of the Obs are used as xerror for the fit.
\n- y (list):\nList of Obs, the dvalues of the Obs are used as yerror for the fit.
\nGenerates a quantile-quantile plot of the fit result which can be used to\ncheck if the residuals of the fit are gaussian distributed.
\n", "signature": "(x, o_y, func, p):", "funcdef": "def"}, "pyerrors.fits.residual_plot": {"fullname": "pyerrors.fits.residual_plot", "modulename": "pyerrors.fits", "qualname": "residual_plot", "kind": "function", "doc": "Generates a plot which compares the fit to the data and displays the corresponding residuals
\n", "signature": "(x, y, func, fit_res):", "funcdef": "def"}, "pyerrors.fits.error_band": {"fullname": "pyerrors.fits.error_band", "modulename": "pyerrors.fits", "qualname": "error_band", "kind": "function", "doc": "Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.
\n", "signature": "(x, func, beta):", "funcdef": "def"}, "pyerrors.fits.ks_test": {"fullname": "pyerrors.fits.ks_test", "modulename": "pyerrors.fits", "qualname": "ks_test", "kind": "function", "doc": "Performs a Kolmogorov\u2013Smirnov test for the p-values of all fit object.
\n\nParameters
\n\n\n
\n", "signature": "(objects=None):", "funcdef": "def"}, "pyerrors.input": {"fullname": "pyerrors.input", "modulename": "pyerrors.input", "kind": "module", "doc": "- objects (list):\nList of fit results to include in the analysis (optional).
\n\n\n
pyerrors
includes aninput
submodule in which input routines and parsers for the output of various numerical programs are contained.Jackknife samples
\n\nFor comparison with other analysis workflows
\n"}, "pyerrors.input.bdio": {"fullname": "pyerrors.input.bdio", "modulename": "pyerrors.input.bdio", "kind": "module", "doc": "\n"}, "pyerrors.input.bdio.read_ADerrors": {"fullname": "pyerrors.input.bdio.read_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "read_ADerrors", "kind": "function", "doc": "pyerrors
can also generate jackknife samples from anObs
object or import jackknife samples into anObs
object.\nSeepyerrors.obs.Obs.export_jackknife
andpyerrors.obs.import_jackknife
for details.Extract generic MCMC data from a bdio file
\n\nread_ADerrors requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.write_ADerrors": {"fullname": "pyerrors.input.bdio.write_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "write_ADerrors", "kind": "function", "doc": "- file_path -- path to the bdio file
\n- bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
\nWrite Obs to a bdio file according to ADerrors conventions
\n\nread_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(obs_list, file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_mesons": {"fullname": "pyerrors.input.bdio.read_mesons", "modulename": "pyerrors.input.bdio", "qualname": "read_mesons", "kind": "function", "doc": "- file_path -- path to the bdio file
\n- bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
\nExtract mesons data from a bdio file and return it as a dictionary
\n\nThe dictionary can be accessed with a tuple consisting of (type, source_position, kappa1, kappa2)
\n\nread_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_dSdm": {"fullname": "pyerrors.input.bdio.read_dSdm", "modulename": "pyerrors.input.bdio", "qualname": "read_dSdm", "kind": "function", "doc": "- file_path (str):\npath to the bdio file
\n- bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
\n- start (int):\nThe first configuration to be read (default 1)
\n- stop (int):\nThe last configuration to be read (default None)
\n- step (int):\nFixed step size between two measurements (default 1)
\n- alternative_ensemble_name (str):\nManually overwrite ensemble name
\nExtract dSdm data from a bdio file and return it as a dictionary
\n\nThe dictionary can be accessed with a tuple consisting of (type, kappa)
\n\nread_dSdm requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.dobs": {"fullname": "pyerrors.input.dobs", "modulename": "pyerrors.input.dobs", "kind": "module", "doc": "\n"}, "pyerrors.input.dobs.create_pobs_string": {"fullname": "pyerrors.input.dobs.create_pobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_pobs_string", "kind": "function", "doc": "- file_path (str):\npath to the bdio file
\n- bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
\n- start (int):\nThe first configuration to be read (default 1)
\n- stop (int):\nThe last configuration to be read (default None)
\n- step (int):\nFixed step size between two measurements (default 1)
\n- alternative_ensemble_name (str):\nManually overwrite ensemble name
\nExport a list of Obs or structures containing Obs to an xml string\naccording to the Zeuthen pobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(obsl, name, spec='', origin='', symbol=[], enstag=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_pobs": {"fullname": "pyerrors.input.dobs.write_pobs", "modulename": "pyerrors.input.dobs", "qualname": "write_pobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
\nExport a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen pobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tfname,\tname,\tspec='',\torigin='',\tsymbol=[],\tenstag=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_pobs": {"fullname": "pyerrors.input.dobs.read_pobs", "modulename": "pyerrors.input.dobs", "qualname": "read_pobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
\n- fname (str):\nFilename of the output file.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
\n- gz (bool):\nIf True, the output is a gzipped xml. If False, the output is an xml file.
\nImport a list of Obs from an xml.gz file in the Zeuthen pobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(fname, full_output=False, gz=True, separator_insertion=None):", "funcdef": "def"}, "pyerrors.input.dobs.import_dobs_string": {"fullname": "pyerrors.input.dobs.import_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "import_dobs_string", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- separatior_insertion (str or int):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nNone (default): Replica names remain unchanged.
\nImport a list of Obs from a string in the Zeuthen dobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(content, noempty=False, full_output=False, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_dobs": {"fullname": "pyerrors.input.dobs.read_dobs", "modulename": "pyerrors.input.dobs", "qualname": "read_dobs", "kind": "function", "doc": "- content (str):\nXML string containing the data
\n- noemtpy (bool):\nIf True, ensembles with no contribution to the Obs are not included.\nIf False, ensembles are included as written in the file, possibly with vanishing entries.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
\nImport a list of Obs from an xml.gz file in the Zeuthen dobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(\tfname,\tnoempty=False,\tfull_output=False,\tgz=True,\tseparator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.create_dobs_string": {"fullname": "pyerrors.input.dobs.create_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_dobs_string", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- noemtpy (bool):\nIf True, ensembles with no contribution to the Obs are not included.\nIf False, ensembles are included as written in the file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes XML file.
\n- separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
\nGenerate the string for the export of a list of Obs or structures containing Obs\nto a .xml.gz file according to the Zeuthen dobs format.
\n\nTags are not written or recovered automatically. The separator |is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_dobs": {"fullname": "pyerrors.input.dobs.write_dobs", "modulename": "pyerrors.input.dobs", "qualname": "write_dobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- who (str):\nProvide the name of the person that exports the data.
\n- enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
\nExport a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen dobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tfname,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.hadrons": {"fullname": "pyerrors.input.hadrons", "modulename": "pyerrors.input.hadrons", "kind": "module", "doc": "\n"}, "pyerrors.input.hadrons.read_meson_hd5": {"fullname": "pyerrors.input.hadrons.read_meson_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_meson_hd5", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
\n- fname (str):\nFilename of the output file.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- who (str):\nProvide the name of the person that exports the data.
\n- enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
\n- gz (bool):\nIf True, the output is a gzipped XML. If False, the output is a XML file.
\nRead hadrons meson hdf5 file and extract the meson labeled 'meson'
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_DistillationContraction_hd5": {"fullname": "pyerrors.input.hadrons.read_DistillationContraction_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_DistillationContraction_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- meson (str):\nlabel of the meson to be extracted, standard value meson_0 which\ncorresponds to the pseudoscalar pseudoscalar two-point function.
\n- gammas (tuple of strings):\nInstrad of a meson label one can also provide a tuple of two strings\nindicating the gamma matrices at source and sink.\n(\"Gamma5\", \"Gamma5\") corresponds to the pseudoscalar pseudoscalar\ntwo-point function. The gammas argument dominateds over meson.
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons DistillationContraction hdf5 files in given directory structure
\n\nParameters
\n\n\n
\n", "signature": "(path, ens_id, diagrams=['direct'], idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.Npr_matrix": {"fullname": "pyerrors.input.hadrons.Npr_matrix", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix", "kind": "class", "doc": "- path (str):\npath to the directories to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- diagrams (list):\nList of strings of the diagrams to extract, e.g. [\"direct\", \"box\", \"cross\"].
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nndarray(shape, dtype=float, buffer=None, offset=0,\n strides=None, order=None)
\n\nAn array object represents a multidimensional, homogeneous array\nof fixed-size items. An associated data-type object describes the\nformat of each element in the array (its byte-order, how many bytes it\noccupies in memory, whether it is an integer, a floating point number,\nor something else, etc.)
\n\nArrays should be constructed using
\n\narray
,zeros
orempty
(refer\nto the See Also section below). The parameters given here refer to\na low-level method (ndarray(...)
) for instantiating an array.For more information, refer to the
\n\nnumpy
module and examine the\nmethods and attributes of an array.Parameters
\n\n\n
\n\n- (for the __new__ method; see Notes below)
\n- shape (tuple of ints):\nShape of created array.
\n- dtype (data-type, optional):\nAny object that can be interpreted as a numpy data type.
\n- buffer (object exposing buffer interface, optional):\nUsed to fill the array with data.
\n- offset (int, optional):\nOffset of array data in buffer.
\n- strides (tuple of ints, optional):\nStrides of data in memory.
\n- order ({'C', 'F'}, optional):\nRow-major (C-style) or column-major (Fortran-style) order.
\nAttributes
\n\n\n
\n\n- T (ndarray):\nTranspose of the array.
\n- data (buffer):\nThe array's elements, in memory.
\n- dtype (dtype object):\nDescribes the format of the elements in the array.
\n- flags (dict):\nDictionary containing information related to memory use, e.g.,\n'C_CONTIGUOUS', 'OWNDATA', 'WRITEABLE', etc.
\n- flat (numpy.flatiter object):\nFlattened version of the array as an iterator. The iterator\nallows assignments, e.g.,
\nx.flat = 3
(Seendarray.flat
for\nassignment examples; TODO).- imag (ndarray):\nImaginary part of the array.
\n- real (ndarray):\nReal part of the array.
\n- size (int):\nNumber of elements in the array.
\n- itemsize (int):\nThe memory use of each array element in bytes.
\n- nbytes (int):\nThe total number of bytes required to store the array data,\ni.e.,
\nitemsize * size
.- ndim (int):\nThe array's number of dimensions.
\n- shape (tuple of ints):\nShape of the array.
\n- strides (tuple of ints):\nThe step-size required to move from one element to the next in\nmemory. For example, a contiguous
\n(3, 4)
array of type\nint16
in C-order has strides(8, 2)
. This implies that\nto move from element to element in memory requires jumps of 2 bytes.\nTo move from row-to-row, one needs to jump 8 bytes at a time\n(2 * 4
).- ctypes (ctypes object):\nClass containing properties of the array needed for interaction\nwith ctypes.
\n- base (ndarray):\nIf the array is a view into another array, that array is its
\nbase
\n(unless that array is also a view). Thebase
array is where the\narray data is actually stored.See Also
\n\n\n\n
array
: Construct an array.
\nzeros
: Create an array, each element of which is zero.
\nempty
: Create an array, but leave its allocated memory unchanged (i.e.,\nit contains \"garbage\").
\ndtype
: Create a data-type.
\nnumpy.typing.NDArray
: An ndarray alias :term:generic <generic type>
\nw.r.t. itsdtype.type <numpy.dtype.type>
.Notes
\n\nThere are two modes of creating an array using
\n\n__new__
:\n
\n\n- If
\nbuffer
is None, then onlyshape
,dtype
, andorder
\nare used.- If
\nbuffer
is an object exposing the buffer interface, then\nall keywords are interpreted.No
\n\n__init__
method is needed because the array is fully initialized\nafter the__new__
method.Examples
\n\nThese examples illustrate the low-level
\n\nndarray
constructor. Refer\nto theSee Also
section above for easier ways of constructing an\nndarray.First mode,
\n\nbuffer
is None:\n\n\n\n>>> np.ndarray(shape=(2,2), dtype=float, order='F')\narray([[0.0e+000, 0.0e+000], # random\n [ nan, 2.5e-323]])\n
Second mode:
\n\n\n\n", "bases": "numpy.ndarray"}, "pyerrors.input.hadrons.Npr_matrix.__init__": {"fullname": "pyerrors.input.hadrons.Npr_matrix.__init__", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.__init__", "kind": "function", "doc": "\n", "signature": "()"}, "pyerrors.input.hadrons.Npr_matrix.g5H": {"fullname": "pyerrors.input.hadrons.Npr_matrix.g5H", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.g5H", "kind": "variable", "doc": "\n>>> np.ndarray((2,), buffer=np.array([1,2,3]),\n... offset=np.int_().itemsize,\n... dtype=int) # offset = 1*itemsize, i.e. skip first element\narray([2, 3])\n
Gamma_5 hermitean conjugate
\n\nUses the fact that the propagator is gamma5 hermitean, so just the\nin and out momenta of the propagator are exchanged.
\n"}, "pyerrors.input.hadrons.read_ExternalLeg_hd5": {"fullname": "pyerrors.input.hadrons.read_ExternalLeg_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_ExternalLeg_hd5", "kind": "function", "doc": "Read hadrons ExternalLeg hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Bilinear_hd5": {"fullname": "pyerrors.input.hadrons.read_Bilinear_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Bilinear_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons Bilinear hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Fourquark_hd5": {"fullname": "pyerrors.input.hadrons.read_Fourquark_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Fourquark_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons FourquarkFullyConnected hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None, vertices=['VA', 'AV']):", "funcdef": "def"}, "pyerrors.input.json": {"fullname": "pyerrors.input.json", "modulename": "pyerrors.input.json", "kind": "module", "doc": "\n"}, "pyerrors.input.json.create_json_string": {"fullname": "pyerrors.input.json.create_json_string", "modulename": "pyerrors.input.json", "qualname": "create_json_string", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\n- vertices (list):\nVertex functions to be extracted.
\nGenerate the string for the export of a list of Obs or structures containing Obs\nto a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(ol, description='', indent=1):", "funcdef": "def"}, "pyerrors.input.json.dump_to_json": {"fullname": "pyerrors.input.json.dump_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_to_json", "kind": "function", "doc": "- ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\nExport a list of Obs or structures containing Obs to a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(ol, fname, description='', indent=1, gz=True):", "funcdef": "def"}, "pyerrors.input.json.import_json_string": {"fullname": "pyerrors.input.json.import_json_string", "modulename": "pyerrors.input.json", "qualname": "import_json_string", "kind": "function", "doc": "- ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- fname (str):\nFilename of the output file.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\n- gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
\nReconstruct a list of Obs or structures containing Obs from a json string.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.
\n\nParameters
\n\n\n
\n", "signature": "(json_string, verbose=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.load_json": {"fullname": "pyerrors.input.json.load_json", "modulename": "pyerrors.input.json", "qualname": "load_json", "kind": "function", "doc": "- json_string (str):\njson string containing the data.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\nImport a list of Obs or structures containing Obs from a .json(.gz) file.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.
\n\nParameters
\n\n\n
\n", "signature": "(fname, verbose=True, gz=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.dump_dict_to_json": {"fullname": "pyerrors.input.json.dump_dict_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_dict_to_json", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\nExport a dict of Obs or structures containing Obs to a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(od, fname, description='', indent=1, reps='DICTOBS', gz=True):", "funcdef": "def"}, "pyerrors.input.json.load_json_dict": {"fullname": "pyerrors.input.json.load_json_dict", "modulename": "pyerrors.input.json", "qualname": "load_json_dict", "kind": "function", "doc": "- od (dict):\nDict of JSON valid structures and objects that will be exported.\nAt the moment, these objects can be either of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- fname (str):\nFilename of the output file.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\n- reps (str):\nSpecify the structure of the placeholder in exported dict to be reps[0-9]+.
\n- gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
\nImport a dict of Obs or structures containing Obs from a .json(.gz) file.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr
\n\nParameters
\n\n\n
\n", "signature": "(fname, verbose=True, gz=True, full_output=False, reps='DICTOBS'):", "funcdef": "def"}, "pyerrors.input.misc": {"fullname": "pyerrors.input.misc", "modulename": "pyerrors.input.misc", "kind": "module", "doc": "\n"}, "pyerrors.input.misc.read_pbp": {"fullname": "pyerrors.input.misc.read_pbp", "modulename": "pyerrors.input.misc", "qualname": "read_pbp", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\n- reps (str):\nSpecify the structure of the placeholder in imported dict to be reps[0-9]+.
\nRead pbp format from given folder structure. Returns a list of length nrw
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD": {"fullname": "pyerrors.input.openQCD", "modulename": "pyerrors.input.openQCD", "kind": "module", "doc": "\n"}, "pyerrors.input.openQCD.read_rwms": {"fullname": "pyerrors.input.openQCD.read_rwms", "modulename": "pyerrors.input.openQCD", "qualname": "read_rwms", "kind": "function", "doc": "- r_start (list):\nlist which contains the first config to be read for each replicum
\n- r_stop (list):\nlist which contains the last config to be read for each replicum
\nRead rwms format from given folder structure. Returns a list of length nrw
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, version='2.0', names=None, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.extract_t0": {"fullname": "pyerrors.input.openQCD.extract_t0", "modulename": "pyerrors.input.openQCD", "qualname": "extract_t0", "kind": "function", "doc": "- path (str):\npath that contains the data files
\n- prefix (str):\nall files in path that start with prefix are considered as input files.\nMay be used together postfix to consider only special file endings.\nPrefix is ignored, if the keyword 'files' is used.
\n- version (str):\nversion of openQCD, default 2.0
\n- names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
\n- r_start (list):\nlist which contains the first config to be read for each replicum
\n- r_stop (list):\nlist which contains the last config to be read for each replicum
\n- r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
\n- postfix (str):\npostfix of the file to read, e.g. '.ms1' for openQCD-files
\n- files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
\n- print_err (bool):\nPrint additional information that is useful for debugging.
\nExtract t0 from given .ms.dat files. Returns t0 as Obs.
\n\nIt is assumed that all boundary effects have\nsufficiently decayed at x0=xmin.\nThe data around the zero crossing of t^2
\n\n- 0.3\nis fitted with a linear function\nfrom which the exact root is extracted. It is assumed that one measurement is performed for each config.\nIf this is not the case, the resulting idl, as well as the handling\nof r_start, r_stop and r_step is wrong and the user has to correct\nthis in the resulting observable.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop": {"fullname": "pyerrors.input.openQCD.read_qtop", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop", "kind": "function", "doc": "- path (str):\nPath to .ms.dat files
\n- prefix (str):\nEnsemble prefix
\n- dtr_read (int):\nDetermines how many trajectories should be skipped\nwhen reading the ms.dat files.\nCorresponds to dtr_cnfg / dtr_ms in the openQCD input file.
\n- xmin (int):\nFirst timeslice where the boundary\neffects have sufficiently decayed.
\n- spatial_extent (int):\nspatial extent of the lattice, required for normalization.
\n- fit_range (int):\nNumber of data points left and right of the zero\ncrossing to be included in the linear fit. (Default: 5)
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
\n- plaquette (bool):\nIf true extract the plaquette estimate of t0 instead.
\n- names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
\n- files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
\n- plot_fit (bool):\nIf true, the fit for the extraction of t0 is shown together with the data.
\n- assume_thermalization (bool):\nIf True: If the first record divided by the distance between two measurements is larger than\n1, it is assumed that this is due to thermalization and the first measurement belongs\nto the first config (default).\nIf False: The config numbers are assumed to be traj_number // difference
\nRead the topologial charge based on openQCD gradient flow measurements.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, dtr_cnfg=1, version='openQCD', **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_gf_coupling": {"fullname": "pyerrors.input.openQCD.read_gf_coupling", "modulename": "pyerrors.input.openQCD", "qualname": "read_gf_coupling", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files. - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- version (str):\nEither openQCD or sfqcd, depending on the data.
\n- L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
\n- integer_charge (bool):\nIf True, the charge is rounded towards the nearest integer on each config.
\nRead the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.
\n\nNote: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.qtop_projection": {"fullname": "pyerrors.input.openQCD.qtop_projection", "modulename": "pyerrors.input.openQCD", "qualname": "qtop_projection", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files. - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
\n- postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
\nReturns the projection to the topological charge sector defined by target.
\n\nParameters
\n\n\n
\n", "signature": "(qtop, target=0):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop_sector": {"fullname": "pyerrors.input.openQCD.read_qtop_sector", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop_sector", "kind": "function", "doc": "- path (Obs):\nTopological charge.
\n- target (int):\nSpecifies the topological sector to be reweighted to (default 0)
\nConstructs reweighting factors to a specified topological sector.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, target=0, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_ms5_xsf": {"fullname": "pyerrors.input.openQCD.read_ms5_xsf", "modulename": "pyerrors.input.openQCD", "qualname": "read_ms5_xsf", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L
\n- target (int):\nSpecifies the topological sector to be reweighted to (default 0)
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of trajectories\nbetween two configs.\nif it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- version (str):\nversion string of the openQCD (sfqcd) version used to create\nthe ensemble. Default is 2.0. May also be set to sfqcd.
\n- L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
\n- r_start (list):\noffset of the first ensemble, making it easier to match\nlater on with other Obs
\n- r_stop (list):\nlast configurations that need to be read (per replicum)
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
\nRead data from files in the specified directory with the specified prefix and quark combination extension, and return a
\n\nCorr
object containing the data.Parameters
\n\n\n
\n\n- path (str):\nThe directory to search for the files in.
\n- prefix (str):\nThe prefix to match the files against.
\n- qc (str):\nThe quark combination extension to match the files against.
\n- corr (str):\nThe correlator to extract data for.
\n- sep (str, optional):\nThe separator to use when parsing the replika names.
\n- \n
**kwargs: Additional keyword arguments. The following keyword arguments are recognized:
\n\n\n
- names (List[str]): A list of names to use for the replicas.
\nReturns
\n\n\n
\n\n- Corr: A complex valued
\nCorr
object containing the data read from the files. In case of boudary to bulk correlators.- or
\n- CObs: A complex valued
\nCObs
object containing the data read from the files. In case of boudary to boundary correlators.Raises
\n\n\n
\n", "signature": "(path, prefix, qc, corr, sep='r', **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas": {"fullname": "pyerrors.input.pandas", "modulename": "pyerrors.input.pandas", "kind": "module", "doc": "\n"}, "pyerrors.input.pandas.to_sql": {"fullname": "pyerrors.input.pandas.to_sql", "modulename": "pyerrors.input.pandas", "qualname": "to_sql", "kind": "function", "doc": "- FileNotFoundError: If no files matching the specified prefix and quark combination extension are found in the specified directory.
\n- IOError: If there is an error reading a file.
\n- struct.error: If there is an error unpacking binary data.
\nWrite DataFrame including Obs or Corr valued columns to sqlite database.
\n\nParameters
\n\n\n
\n", "signature": "(df, table_name, db, if_exists='fail', gz=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.read_sql": {"fullname": "pyerrors.input.pandas.read_sql", "modulename": "pyerrors.input.pandas", "qualname": "read_sql", "kind": "function", "doc": "- df (pandas.DataFrame):\nDataframe to be written to the database.
\n- table_name (str):\nName of the table in the database.
\n- db (str):\nPath to the sqlite database.
\n- if exists (str):\nHow to behave if table already exists. Options 'fail', 'replace', 'append'.
\n- gz (bool):\nIf True the json strings are gzipped.
\nExecute SQL query on sqlite database and obtain DataFrame including Obs or Corr valued columns.
\n\nParameters
\n\n\n
\n", "signature": "(sql, db, auto_gamma=False, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.dump_df": {"fullname": "pyerrors.input.pandas.dump_df", "modulename": "pyerrors.input.pandas", "qualname": "dump_df", "kind": "function", "doc": "- sql (str):\nSQL query to be executed.
\n- db (str):\nPath to the sqlite database.
\n- auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
\nExports a pandas DataFrame containing Obs valued columns to a (gzipped) csv file.
\n\nBefore making use of pandas to_csv functionality Obs objects are serialized via the standardized\njson format of pyerrors.
\n\nParameters
\n\n\n
\n", "signature": "(df, fname, gz=True):", "funcdef": "def"}, "pyerrors.input.pandas.load_df": {"fullname": "pyerrors.input.pandas.load_df", "modulename": "pyerrors.input.pandas", "qualname": "load_df", "kind": "function", "doc": "- df (pandas.DataFrame):\nDataframe to be dumped to a file.
\n- fname (str):\nFilename of the output file.
\n- gz (bool):\nIf True, the output is a gzipped csv file. If False, the output is a csv file.
\nImports a pandas DataFrame from a csv.(gz) file in which Obs objects are serialized as json strings.
\n\nParameters
\n\n\n
\n", "signature": "(fname, auto_gamma=False, gz=True):", "funcdef": "def"}, "pyerrors.input.sfcf": {"fullname": "pyerrors.input.sfcf", "modulename": "pyerrors.input.sfcf", "kind": "module", "doc": "\n"}, "pyerrors.input.sfcf.read_sfcf": {"fullname": "pyerrors.input.sfcf.read_sfcf", "modulename": "pyerrors.input.sfcf", "qualname": "read_sfcf", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\nRead sfcf c format from given folder structure.
\n\nParameters
\n\n\n
\n", "signature": "(\tpath,\tprefix,\tname,\tquarks='.*',\tcorr_type='bi',\tnoffset=0,\twf=0,\twf2=0,\tversion='1.0c',\tcfg_separator='n',\t**kwargs):", "funcdef": "def"}, "pyerrors.input.utils": {"fullname": "pyerrors.input.utils", "modulename": "pyerrors.input.utils", "kind": "module", "doc": "- path (str):\nPath to the sfcf files.
\n- prefix (str):\nPrefix of the sfcf files.
\n- name (str):\nName of the correlation function to read.
\n- quarks (str):\nLabel of the quarks used in the sfcf input file. e.g. \"quark quark\"\nfor version 0.0 this does NOT need to be given with the typical \" - \"\nthat is present in the output file,\nthis is done automatically for this version
\n- corr_type (str):\nType of correlation function to read. Can be\n
\n\n
- 'bi' for boundary-inner
\n- 'bb' for boundary-boundary
\n- 'bib' for boundary-inner-boundary
\n- noffset (int):\nOffset of the source (only relevant when wavefunctions are used)
\n- wf (int):\nID of wave function
\n- wf2 (int):\nID of the second wavefunction\n(only relevant for boundary-to-boundary correlation functions)
\n- im (bool):\nif True, read imaginary instead of real part\nof the correlation function.
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
\n- ens_name (str):\nreplaces the name of the ensemble
\n- version (str):\nversion of SFCF, with which the measurement was done.\nif the compact output option (-c) was specified,\nappend a \"c\" to the version (e.g. \"1.0c\")\nif the append output option (-a) was specified,\nappend an \"a\" to the version
\n- cfg_separator (str):\nString that separates the ensemble identifier from the configuration number (default 'n').
\n- replica (list):\nlist of replica to be read, default is all
\n- files (list):\nlist of files to be read per replica, default is all.\nfor non-compact output format, hand the folders to be read here.
\n- check_configs:: list of list of supposed configs, eg. [range(1,1000)]\nfor one replicum with 1000 configs
\nUtilities for the input
\n"}, "pyerrors.input.utils.check_idl": {"fullname": "pyerrors.input.utils.check_idl", "modulename": "pyerrors.input.utils", "qualname": "check_idl", "kind": "function", "doc": "Checks if list of configurations is contained in an idl
\n\nParameters
\n\n\n
\n", "signature": "(idl, che):", "funcdef": "def"}, "pyerrors.linalg": {"fullname": "pyerrors.linalg", "modulename": "pyerrors.linalg", "kind": "module", "doc": "\n"}, "pyerrors.linalg.matmul": {"fullname": "pyerrors.linalg.matmul", "modulename": "pyerrors.linalg", "qualname": "matmul", "kind": "function", "doc": "- idl (range or list):\nidl of the current replicum
\n- che (list):\nlist of configurations to be checked against
\nMatrix multiply all operands.
\n\nParameters
\n\n\n
\n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.jack_matmul": {"fullname": "pyerrors.linalg.jack_matmul", "modulename": "pyerrors.linalg", "qualname": "jack_matmul", "kind": "function", "doc": "- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\n- This implementation is faster compared to standard multiplication via the @ operator.
\nMatrix multiply both operands making use of the jackknife approximation.
\n\nParameters
\n\n\n
\n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.einsum": {"fullname": "pyerrors.linalg.einsum", "modulename": "pyerrors.linalg", "qualname": "einsum", "kind": "function", "doc": "- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\n- For large matrices this is considerably faster compared to matmul.
\nWrapper for numpy.einsum
\n\nParameters
\n\n\n
\n", "signature": "(subscripts, *operands):", "funcdef": "def"}, "pyerrors.linalg.inv": {"fullname": "pyerrors.linalg.inv", "modulename": "pyerrors.linalg", "qualname": "inv", "kind": "function", "doc": "- subscripts (str):\nSubscripts for summation (see numpy documentation for details)
\n- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\nInverse of Obs or CObs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.cholesky": {"fullname": "pyerrors.linalg.cholesky", "modulename": "pyerrors.linalg", "qualname": "cholesky", "kind": "function", "doc": "Cholesky decomposition of Obs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.det": {"fullname": "pyerrors.linalg.det", "modulename": "pyerrors.linalg", "qualname": "det", "kind": "function", "doc": "Determinant of Obs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.eigh": {"fullname": "pyerrors.linalg.eigh", "modulename": "pyerrors.linalg", "qualname": "eigh", "kind": "function", "doc": "Computes the eigenvalues and eigenvectors of a given hermitian matrix of Obs according to np.linalg.eigh.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.eig": {"fullname": "pyerrors.linalg.eig", "modulename": "pyerrors.linalg", "qualname": "eig", "kind": "function", "doc": "Computes the eigenvalues of a given matrix of Obs according to np.linalg.eig.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.pinv": {"fullname": "pyerrors.linalg.pinv", "modulename": "pyerrors.linalg", "qualname": "pinv", "kind": "function", "doc": "Computes the Moore-Penrose pseudoinverse of a matrix of Obs.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.svd": {"fullname": "pyerrors.linalg.svd", "modulename": "pyerrors.linalg", "qualname": "svd", "kind": "function", "doc": "Computes the singular value decomposition of a matrix of Obs.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.misc": {"fullname": "pyerrors.misc", "modulename": "pyerrors.misc", "kind": "module", "doc": "\n"}, "pyerrors.misc.dump_object": {"fullname": "pyerrors.misc.dump_object", "modulename": "pyerrors.misc", "qualname": "dump_object", "kind": "function", "doc": "Dump object into pickle file.
\n\nParameters
\n\n\n
\n", "signature": "(obj, name, **kwargs):", "funcdef": "def"}, "pyerrors.misc.load_object": {"fullname": "pyerrors.misc.load_object", "modulename": "pyerrors.misc", "qualname": "load_object", "kind": "function", "doc": "- obj (object):\nobject to be saved in the pickle file
\n- name (str):\nname of the file
\n- path (str):\nspecifies a custom path for the file (default '.')
\nLoad object from pickle file.
\n\nParameters
\n\n\n
\n", "signature": "(path):", "funcdef": "def"}, "pyerrors.misc.pseudo_Obs": {"fullname": "pyerrors.misc.pseudo_Obs", "modulename": "pyerrors.misc", "qualname": "pseudo_Obs", "kind": "function", "doc": "- path (str):\npath to the file
\nGenerate an Obs object with given value, dvalue and name for test purposes
\n\nParameters
\n\n\n
\n", "signature": "(value, dvalue, name, samples=1000):", "funcdef": "def"}, "pyerrors.misc.gen_correlated_data": {"fullname": "pyerrors.misc.gen_correlated_data", "modulename": "pyerrors.misc", "qualname": "gen_correlated_data", "kind": "function", "doc": "- value (float):\ncentral value of the Obs to be generated.
\n- dvalue (float):\nerror of the Obs to be generated.
\n- name (str):\nname of the ensemble for which the Obs is to be generated.
\n- samples (int):\nnumber of samples for the Obs (default 1000).
\nGenerate observables with given covariance and autocorrelation times.
\n\nParameters
\n\n\n
\n", "signature": "(means, cov, name, tau=0.5, samples=1000):", "funcdef": "def"}, "pyerrors.mpm": {"fullname": "pyerrors.mpm", "modulename": "pyerrors.mpm", "kind": "module", "doc": "\n"}, "pyerrors.mpm.matrix_pencil_method": {"fullname": "pyerrors.mpm.matrix_pencil_method", "modulename": "pyerrors.mpm", "qualname": "matrix_pencil_method", "kind": "function", "doc": "- means (list):\nlist containing the mean value of each observable.
\n- cov (numpy.ndarray):\ncovariance matrix for the data to be generated.
\n- name (str):\nensemble name for the data to be geneated.
\n- tau (float or list):\ncan either be a real number or a list with an entry for\nevery dataset.
\n- samples (int):\nnumber of samples to be generated for each observable.
\nMatrix pencil method to extract k energy levels from data
\n\nImplementation of the matrix pencil method based on\neq. (2.17) of Y. Hua, T. K. Sarkar, IEEE Trans. Acoust. 38, 814-824 (1990)
\n\nParameters
\n\n\n
\n", "signature": "(corrs, k=1, p=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs": {"fullname": "pyerrors.obs", "modulename": "pyerrors.obs", "kind": "module", "doc": "\n"}, "pyerrors.obs.Obs": {"fullname": "pyerrors.obs.Obs", "modulename": "pyerrors.obs", "qualname": "Obs", "kind": "class", "doc": "- data (list):\ncan be a list of Obs for the analysis of a single correlator, or a list of lists\nof Obs if several correlators are to analyzed at once.
\n- k (int):\nNumber of states to extract (default 1).
\n- p (int):\nmatrix pencil parameter which filters noise. The optimal value is expected between\nlen(data)/3 and 2*len(data)/3. The computation is more expensive the closer p is\nto len(data)/2 but could possibly suppress more noise (default len(data)//2).
\nClass for a general observable.
\n\nInstances of Obs are the basic objects of a pyerrors error analysis.\nThey are initialized with a list which contains arrays of samples for\ndifferent ensembles/replica and another list of same length which contains\nthe names of the ensembles/replica. Mathematical operations can be\nperformed on instances. The result is another instance of Obs. The error of\nan instance can be computed with the gamma_method. Also contains additional\nmethods for output and visualization of the error calculation.
\n\nAttributes
\n\n\n
\n"}, "pyerrors.obs.Obs.__init__": {"fullname": "pyerrors.obs.Obs.__init__", "modulename": "pyerrors.obs", "qualname": "Obs.__init__", "kind": "function", "doc": "- S_global (float):\nStandard value for S (default 2.0)
\n- S_dict (dict):\nDictionary for S values. If an entry for a given ensemble\nexists this overwrites the standard value for that ensemble.
\n- tau_exp_global (float):\nStandard value for tau_exp (default 0.0)
\n- tau_exp_dict (dict):\nDictionary for tau_exp values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
\n- N_sigma_global (float):\nStandard value for N_sigma (default 1.0)
\n- N_sigma_dict (dict):\nDictionary for N_sigma values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
\nInitialize Obs object.
\n\nParameters
\n\n\n
\n", "signature": "(samples, names, idl=None, **kwargs)"}, "pyerrors.obs.Obs.gamma_method": {"fullname": "pyerrors.obs.Obs.gamma_method", "modulename": "pyerrors.obs", "qualname": "Obs.gamma_method", "kind": "function", "doc": "- samples (list):\nlist of numpy arrays containing the Monte Carlo samples
\n- names (list):\nlist of strings labeling the individual samples
\n- idl (list, optional):\nlist of ranges or lists on which the samples are defined
\nEstimate the error and related properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.gm": {"fullname": "pyerrors.obs.Obs.gm", "modulename": "pyerrors.obs", "qualname": "Obs.gm", "kind": "function", "doc": "- S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
\n- tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
\n- N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
\n- fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
\nEstimate the error and related properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.details": {"fullname": "pyerrors.obs.Obs.details", "modulename": "pyerrors.obs", "qualname": "Obs.details", "kind": "function", "doc": "- S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
\n- tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
\n- N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
\n- fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
\nOutput detailed properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, ens_content=True):", "funcdef": "def"}, "pyerrors.obs.Obs.reweight": {"fullname": "pyerrors.obs.Obs.reweight", "modulename": "pyerrors.obs", "qualname": "Obs.reweight", "kind": "function", "doc": "- ens_content (bool):\nprint details about the ensembles and replica if true.
\nReweight the obs with given rewighting factors.
\n\nParameters
\n\n\n
\n", "signature": "(self, weight):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero_within_error": {"fullname": "pyerrors.obs.Obs.is_zero_within_error", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero_within_error", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
\nChecks whether the observable is zero within 'sigma' standard errors.
\n\nParameters
\n\n\n
\n", "signature": "(self, sigma=1):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero": {"fullname": "pyerrors.obs.Obs.is_zero", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero", "kind": "function", "doc": "- sigma (int):\nNumber of standard errors used for the check.
\n- Works only properly when the gamma method was run.
\nChecks whether the observable is zero within a given tolerance.
\n\nParameters
\n\n\n
\n", "signature": "(self, atol=1e-10):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_tauint": {"fullname": "pyerrors.obs.Obs.plot_tauint", "modulename": "pyerrors.obs", "qualname": "Obs.plot_tauint", "kind": "function", "doc": "- atol (float):\nAbsolute tolerance (for details see numpy documentation).
\nPlot integrated autocorrelation time for each ensemble.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rho": {"fullname": "pyerrors.obs.Obs.plot_rho", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rho", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nPlot normalized autocorrelation function time for each ensemble.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rep_dist": {"fullname": "pyerrors.obs.Obs.plot_rep_dist", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rep_dist", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nPlot replica distribution for each ensemble with more than one replicum.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_history": {"fullname": "pyerrors.obs.Obs.plot_history", "modulename": "pyerrors.obs", "qualname": "Obs.plot_history", "kind": "function", "doc": "Plot derived Monte Carlo history for each ensemble
\n\nParameters
\n\n\n
\n", "signature": "(self, expand=True):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_piechart": {"fullname": "pyerrors.obs.Obs.plot_piechart", "modulename": "pyerrors.obs", "qualname": "Obs.plot_piechart", "kind": "function", "doc": "- expand (bool):\nshow expanded history for irregular Monte Carlo chains (default: True).
\nPlot piechart which shows the fractional contribution of each\nensemble to the error and returns a dictionary containing the fractions.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.dump": {"fullname": "pyerrors.obs.Obs.dump", "modulename": "pyerrors.obs", "qualname": "Obs.dump", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nDump the Obs to a file 'name' of chosen format.
\n\nParameters
\n\n\n
\n", "signature": "(self, filename, datatype='json.gz', description='', **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.export_jackknife": {"fullname": "pyerrors.obs.Obs.export_jackknife", "modulename": "pyerrors.obs", "qualname": "Obs.export_jackknife", "kind": "function", "doc": "- filename (str):\nname of the file to be saved.
\n- datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
\n- description (str):\nDescription for output file, only relevant for json.gz format.
\n- path (str):\nspecifies a custom path for the file (default '.')
\nExport jackknife samples from the Obs
\n\nReturns
\n\n\n
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sqrt": {"fullname": "pyerrors.obs.Obs.sqrt", "modulename": "pyerrors.obs", "qualname": "Obs.sqrt", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.log": {"fullname": "pyerrors.obs.Obs.log", "modulename": "pyerrors.obs", "qualname": "Obs.log", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.exp": {"fullname": "pyerrors.obs.Obs.exp", "modulename": "pyerrors.obs", "qualname": "Obs.exp", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sin": {"fullname": "pyerrors.obs.Obs.sin", "modulename": "pyerrors.obs", "qualname": "Obs.sin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cos": {"fullname": "pyerrors.obs.Obs.cos", "modulename": "pyerrors.obs", "qualname": "Obs.cos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tan": {"fullname": "pyerrors.obs.Obs.tan", "modulename": "pyerrors.obs", "qualname": "Obs.tan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsin": {"fullname": "pyerrors.obs.Obs.arcsin", "modulename": "pyerrors.obs", "qualname": "Obs.arcsin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccos": {"fullname": "pyerrors.obs.Obs.arccos", "modulename": "pyerrors.obs", "qualname": "Obs.arccos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctan": {"fullname": "pyerrors.obs.Obs.arctan", "modulename": "pyerrors.obs", "qualname": "Obs.arctan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sinh": {"fullname": "pyerrors.obs.Obs.sinh", "modulename": "pyerrors.obs", "qualname": "Obs.sinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cosh": {"fullname": "pyerrors.obs.Obs.cosh", "modulename": "pyerrors.obs", "qualname": "Obs.cosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tanh": {"fullname": "pyerrors.obs.Obs.tanh", "modulename": "pyerrors.obs", "qualname": "Obs.tanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsinh": {"fullname": "pyerrors.obs.Obs.arcsinh", "modulename": "pyerrors.obs", "qualname": "Obs.arcsinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccosh": {"fullname": "pyerrors.obs.Obs.arccosh", "modulename": "pyerrors.obs", "qualname": "Obs.arccosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctanh": {"fullname": "pyerrors.obs.Obs.arctanh", "modulename": "pyerrors.obs", "qualname": "Obs.arctanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs": {"fullname": "pyerrors.obs.CObs", "modulename": "pyerrors.obs", "qualname": "CObs", "kind": "class", "doc": "- numpy.ndarray: Returns a numpy array of length N + 1 where N is the number of samples\nfor the given ensemble and replicum. The zeroth entry of the array contains\nthe mean value of the Obs, entries 1 to N contain the N jackknife samples\nderived from the Obs. The current implementation only works for observables\ndefined on exactly one ensemble and replicum. The derived jackknife samples\nshould agree with samples from a full jackknife analysis up to O(1/N).
\nClass for a complex valued observable.
\n"}, "pyerrors.obs.CObs.__init__": {"fullname": "pyerrors.obs.CObs.__init__", "modulename": "pyerrors.obs", "qualname": "CObs.__init__", "kind": "function", "doc": "\n", "signature": "(real, imag=0.0)"}, "pyerrors.obs.CObs.gamma_method": {"fullname": "pyerrors.obs.CObs.gamma_method", "modulename": "pyerrors.obs", "qualname": "CObs.gamma_method", "kind": "function", "doc": "Executes the gamma_method for the real and the imaginary part.
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.CObs.is_zero": {"fullname": "pyerrors.obs.CObs.is_zero", "modulename": "pyerrors.obs", "qualname": "CObs.is_zero", "kind": "function", "doc": "Checks whether both real and imaginary part are zero within machine precision.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs.conjugate": {"fullname": "pyerrors.obs.CObs.conjugate", "modulename": "pyerrors.obs", "qualname": "CObs.conjugate", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.derived_observable": {"fullname": "pyerrors.obs.derived_observable", "modulename": "pyerrors.obs", "qualname": "derived_observable", "kind": "function", "doc": "Construct a derived Obs according to func(data, **kwargs) using automatic differentiation.
\n\nParameters
\n\n\n
\n\n- func (object):\narbitrary function of the form func(data, **kwargs). For the\nautomatic differentiation to work, all numpy functions have to have\nthe autograd wrapper (use 'import autograd.numpy as anp').
\n- data (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
\n- num_grad (bool):\nif True, numerical derivatives are used instead of autograd\n(default False). To control the numerical differentiation the\nkwargs of numdifftools.step_generators.MaxStepGenerator\ncan be used.
\n- man_grad (list):\nmanually supply a list or an array which contains the jacobian\nof func. Use cautiously, supplying the wrong derivative will\nnot be intercepted.
\nNotes
\n\nFor simple mathematical operations it can be practical to use anonymous\nfunctions. For the ratio of two observables one can e.g. use
\n\nnew_obs = derived_observable(lambda x: x[0] / x[1], [obs1, obs2])
\n", "signature": "(func, data, array_mode=False, **kwargs):", "funcdef": "def"}, "pyerrors.obs.reweight": {"fullname": "pyerrors.obs.reweight", "modulename": "pyerrors.obs", "qualname": "reweight", "kind": "function", "doc": "Reweight a list of observables.
\n\nParameters
\n\n\n
\n", "signature": "(weight, obs, **kwargs):", "funcdef": "def"}, "pyerrors.obs.correlate": {"fullname": "pyerrors.obs.correlate", "modulename": "pyerrors.obs", "qualname": "correlate", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- obs (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
\nCorrelate two observables.
\n\nParameters
\n\n\n
\n\n- obs_a (Obs):\nFirst observable
\n- obs_b (Obs):\nSecond observable
\nNotes
\n\nKeep in mind to only correlate primary observables which have not been reweighted\nyet. The reweighting has to be applied after correlating the observables.\nCurrently only works if ensembles are identical (this is not strictly necessary).
\n", "signature": "(obs_a, obs_b):", "funcdef": "def"}, "pyerrors.obs.covariance": {"fullname": "pyerrors.obs.covariance", "modulename": "pyerrors.obs", "qualname": "covariance", "kind": "function", "doc": "Calculates the error covariance matrix of a set of observables.
\n\nWARNING: This function should be used with care, especially for observables with support on multiple\n ensembles with differing autocorrelations. See the notes below for details.
\n\nThe gamma method has to be applied first to all observables.
\n\nParameters
\n\n\n
\n\n- obs (list or numpy.ndarray):\nList or one dimensional array of Obs
\n- visualize (bool):\nIf True plots the corresponding normalized correlation matrix (default False).
\n- correlation (bool):\nIf True the correlation matrix instead of the error covariance matrix is returned (default False).
\n- smooth (None or int):\nIf smooth is an integer 'E' between 2 and the dimension of the matrix minus 1 the eigenvalue\nsmoothing procedure of hep-lat/9412087 is applied to the correlation matrix which leaves the\nlargest E eigenvalues essentially unchanged and smoothes the smaller eigenvalues to avoid extremely\nsmall ones.
\nNotes
\n\nThe error covariance is defined such that it agrees with the squared standard error for two identical observables\n$$\\operatorname{cov}(a,a)=\\sum_{s=1}^N\\delta_a^s\\delta_a^s/N^2=\\Gamma_{aa}(0)/N=\\operatorname{var}(a)/N=\\sigma_a^2$$\nin the absence of autocorrelation.\nThe error covariance is estimated by calculating the correlation matrix assuming no autocorrelation and then rescaling the correlation matrix by the full errors including the previous gamma method estimate for the autocorrelation of the observables. The covariance at windowsize 0 is guaranteed to be positive semi-definite\n$$\\sum_{i,j}v_i\\Gamma_{ij}(0)v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i,j}v_i\\delta_i^s\\delta_j^s v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i}|v_i\\delta_i^s|^2\\geq 0\\,,$$ for every $v\\in\\mathbb{R}^M$, while such an identity does not hold for larger windows/lags.\nFor observables defined on a single ensemble our approximation is equivalent to assuming that the integrated autocorrelation time of an off-diagonal element is equal to the geometric mean of the integrated autocorrelation times of the corresponding diagonal elements.\n$$\\tau_{\\mathrm{int}, ij}=\\sqrt{\\tau_{\\mathrm{int}, i}\\times \\tau_{\\mathrm{int}, j}}$$\nThis construction ensures that the estimated covariance matrix is positive semi-definite (up to numerical rounding errors).
\n", "signature": "(obs, visualize=False, correlation=False, smooth=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs.import_jackknife": {"fullname": "pyerrors.obs.import_jackknife", "modulename": "pyerrors.obs", "qualname": "import_jackknife", "kind": "function", "doc": "Imports jackknife samples and returns an Obs
\n\nParameters
\n\n\n
\n", "signature": "(jacks, name, idl=None):", "funcdef": "def"}, "pyerrors.obs.merge_obs": {"fullname": "pyerrors.obs.merge_obs", "modulename": "pyerrors.obs", "qualname": "merge_obs", "kind": "function", "doc": "- jacks (numpy.ndarray):\nnumpy array containing the mean value as zeroth entry and\nthe N jackknife samples as first to Nth entry.
\n- name (str):\nname of the ensemble the samples are defined on.
\nCombine all observables in list_of_obs into one new observable
\n\nParameters
\n\n\n
\n\n- list_of_obs (list):\nlist of the Obs object to be combined
\nNotes
\n\nIt is not possible to combine obs which are based on the same replicum
\n", "signature": "(list_of_obs):", "funcdef": "def"}, "pyerrors.obs.cov_Obs": {"fullname": "pyerrors.obs.cov_Obs", "modulename": "pyerrors.obs", "qualname": "cov_Obs", "kind": "function", "doc": "Create an Obs based on mean(s) and a covariance matrix
\n\nParameters
\n\n\n
\n", "signature": "(means, cov, name, grad=None):", "funcdef": "def"}, "pyerrors.roots": {"fullname": "pyerrors.roots", "modulename": "pyerrors.roots", "kind": "module", "doc": "\n"}, "pyerrors.roots.find_root": {"fullname": "pyerrors.roots.find_root", "modulename": "pyerrors.roots", "qualname": "find_root", "kind": "function", "doc": "- mean (list of floats or float):\nN mean value(s) of the new Obs
\n- cov (list or array):\n2d (NxN) Covariance matrix, 1d diagonal entries or 0d covariance
\n- name (str):\nidentifier for the covariance matrix
\n- grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
\nFinds the root of the function func(x, d) where d is an
\n\nObs
.Parameters
\n\n\n
\n\n- d (Obs):\nObs passed to the function.
\n- \n
func (object):\nFunction to be minimized. Any numpy functions have to use the autograd.numpy wrapper.\nExample:
\n\n\n\nimport autograd.numpy as anp\ndef root_func(x, d):\n return anp.exp(-x ** 2) - d\n
- \n
guess (float):\nInitial guess for the minimization.
Returns
\n\n\n
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\nObs
valued root of the function.What is pyerrors?
\n\n\n\n
pyerrors
is a python package for error computation and propagation of Markov chain Monte Carlo data.\nIt is based on the gamma method arXiv:hep-lat/0306017. Some of its features are:\n
\n\n- automatic differentiation for exact linear error propagation as suggested in arXiv:1809.01289 (partly based on the autograd package).
\n- treatment of slow modes in the simulation as suggested in arXiv:1009.5228.
\n- coherent error propagation for data from different Markov chains.
\n- non-linear fits with x- and y-errors and exact linear error propagation based on automatic differentiation as introduced in arXiv:1809.01289.
\n- real and complex matrix operations and their error propagation based on automatic differentiation (Matrix inverse, Cholesky decomposition, calculation of eigenvalues and eigenvectors, singular value decomposition...).
\nMore detailed examples can found in the GitHub repository
\n\n.
If you use
\n\npyerrors
for research that leads to a publication please consider citing:\n
\n\n- Fabian Joswig, Simon Kuberski, Justus T. Kuhlmann, Jan Neuendorf, pyerrors: a python framework for error analysis of Monte Carlo data. [arXiv:2209.14371 [hep-lat]].
\n- Ulli Wolff, Monte Carlo errors with less errors. Comput.Phys.Commun. 156 (2004) 143-153, Comput.Phys.Commun. 176 (2007) 383 (erratum).
\n- Alberto Ramos, Automatic differentiation for error analysis of Monte Carlo data. Comput.Phys.Commun. 238 (2019) 19-35.
\nand
\n\n\n
\n\n- Stefan Schaefer, Rainer Sommer, Francesco Virotta, Critical slowing down and error analysis in lattice QCD simulations. Nucl.Phys.B 845 (2011) 93-119.
\nwhere applicable.
\n\nThere exist similar publicly available implementations of gamma method error analysis suites in Fortran, Julia and Python.
\n\nBasic example
\n\n\n\n\n\nimport numpy as np\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name']) # Initialize an Obs object\nmy_new_obs = 2 * np.log(my_obs) / my_obs ** 2 # Construct derived Obs object\nmy_new_obs.gamma_method() # Estimate the statistical error\nprint(my_new_obs) # Print the result to stdout\n> 0.31498(72)\n
The
\n\nObs
class\n\n
pyerrors
introduces a new datatype,Obs
, which simplifies error propagation and estimation for auto- and cross-correlated data.\nAnObs
object can be initialized with two arguments, the first is a list containing the samples for an observable from a Monte Carlo chain.\nThe samples can either be provided as python list or as numpy array.\nThe second argument is a list containing the names of the respective Monte Carlo chains as strings. These strings uniquely identify a Monte Carlo chain/ensemble.\n\n\n\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name'])\n
Error propagation
\n\nWhen performing mathematical operations on
\n\nObs
objects the correct error propagation is intrinsically taken care of using a first order Taylor expansion\n$$\\delta_f^i=\\sum_\\alpha \\bar{f}_\\alpha \\delta_\\alpha^i\\,,\\quad \\delta_\\alpha^i=a_\\alpha^i-\\bar{a}_\\alpha\\,,$$\nas introduced in arXiv:hep-lat/0306017.\nThe required derivatives $\\bar{f}_\\alpha$ are evaluated up to machine precision via automatic differentiation as suggested in arXiv:1809.01289.The
\n\nObs
class is designed such that mathematical numpy functions can be used onObs
just as for regular floats.\n\n\n\nimport numpy as np\nimport pyerrors as pe\n\nmy_obs1 = pe.Obs([samples1], ['ensemble_name'])\nmy_obs2 = pe.Obs([samples2], ['ensemble_name'])\n\nmy_sum = my_obs1 + my_obs2\n\nmy_m_eff = np.log(my_obs1 / my_obs2)\n\niamzero = my_m_eff - my_m_eff\n# Check that value and fluctuations are zero within machine precision\nprint(iamzero == 0.0)\n> True\n
Error estimation
\n\nThe error estimation within
\n\npyerrors
is based on the gamma method introduced in arXiv:hep-lat/0306017.\nAfter having arrived at the derived quantity of interest thegamma_method
can be called as detailed in the following example.\n\n\n\nmy_sum.gamma_method()\nprint(my_sum)\n> 1.70(57)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 5.72046658e-01 +/- 7.56746598e-02 (33.650%)\n> t_int 2.71422900e+00 +/- 6.40320983e-01 S = 2.00\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
We use the following definition of the integrated autocorrelation time established in Madras & Sokal 1988\n$$\\tau_\\mathrm{int}=\\frac{1}{2}+\\sum_{t=1}^{W}\\rho(t)\\geq \\frac{1}{2}\\,.$$\nThe window $W$ is determined via the automatic windowing procedure described in arXiv:hep-lat/0306017.\nThe standard value for the parameter $S$ of this automatic windowing procedure is $S=2$. Other values for $S$ can be passed to the
\n\ngamma_method
as parameter.\n\n\n\nmy_sum.gamma_method(S=3.0)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 6.30675201e-01 +/- 1.04585650e-01 (37.099%)\n> t_int 3.29909703e+00 +/- 9.77310102e-01 S = 3.00\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
The integrated autocorrelation time $\\tau_\\mathrm{int}$ and the autocorrelation function $\\rho(W)$ can be monitored via the methods
\n\npyerrors.obs.Obs.plot_tauint
andpyerrors.obs.Obs.plot_rho
.If the parameter $S$ is set to zero it is assumed that the dataset does not exhibit any autocorrelation and the window size is chosen to be zero.\nIn this case the error estimate is identical to the sample standard error.
\n\nExponential tails
\n\nSlow modes in the Monte Carlo history can be accounted for by attaching an exponential tail to the autocorrelation function $\\rho$ as suggested in arXiv:1009.5228. The longest autocorrelation time in the history, $\\tau_\\mathrm{exp}$, can be passed to the
\n\ngamma_method
as parameter. In this case the automatic windowing procedure is vacated and the parameter $S$ does not affect the error estimate.\n\n\n\nmy_sum.gamma_method(tau_exp=7.2)\nmy_sum.details()\n> Result 1.70000000e+00 +/- 6.28097762e-01 +/- 5.79077524e-02 (36.947%)\n> t_int 3.27218667e+00 +/- 7.99583654e-01 tau_exp = 7.20, N_sigma = 1\n> 1000 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
For the full API see
\n\npyerrors.obs.Obs.gamma_method
.Multiple ensembles/replica
\n\nError propagation for multiple ensembles (Markov chains with different simulation parameters) is handled automatically. Ensembles are uniquely identified by their
\n\nname
.\n\n\n\nobs1 = pe.Obs([samples1], ['ensemble1'])\nobs2 = pe.Obs([samples2], ['ensemble2'])\n\nmy_sum = obs1 + obs2\nmy_sum.details()\n> Result 2.00697958e+00\n> 1500 samples in 2 ensembles:\n> \u00b7 Ensemble 'ensemble1' : 1000 configurations (from 1 to 1000)\n> \u00b7 Ensemble 'ensemble2' : 500 configurations (from 1 to 500)\n
\n\n
pyerrors
identifies multiple replica (independent Markov chains with identical simulation parameters) by the vertical bar|
in the name of the data set.\n\n\n\nobs1 = pe.Obs([samples1], ['ensemble1|r01'])\nobs2 = pe.Obs([samples2], ['ensemble1|r02'])\n\n> my_sum = obs1 + obs2\n> my_sum.details()\n> Result 2.00697958e+00\n> 1500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1'\n> \u00b7 Replicum 'r01' : 1000 configurations (from 1 to 1000)\n> \u00b7 Replicum 'r02' : 500 configurations (from 1 to 500)\n
Error estimation for multiple ensembles
\n\nIn order to keep track of different error analysis parameters for different ensembles one can make use of global dictionaries as detailed in the following example.
\n\n\n\n\n\npe.Obs.S_dict['ensemble1'] = 2.5\npe.Obs.tau_exp_dict['ensemble2'] = 8.0\npe.Obs.tau_exp_dict['ensemble3'] = 2.0\n
In case the
\n\ngamma_method
is called without any parameters it will use the values specified in the dictionaries for the respective ensembles.\nPassing arguments to thegamma_method
still dominates over the dictionaries.Irregular Monte Carlo chains
\n\n\n\n
Obs
objects defined on irregular Monte Carlo chains can be initialized with the parameteridl
.\n\n\n\n# Observable defined on configurations 20 to 519\nobs1 = pe.Obs([samples1], ['ensemble1'], idl=[range(20, 520)])\nobs1.details()\n> Result 9.98319881e-01\n> 500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 500 configurations (from 20 to 519)\n\n# Observable defined on every second configuration between 5 and 1003\nobs2 = pe.Obs([samples2], ['ensemble1'], idl=[range(5, 1005, 2)])\nobs2.details()\n> Result 9.99100712e-01\n> 500 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 500 configurations (from 5 to 1003 in steps of 2)\n\n# Observable defined on configurations 2, 9, 28, 29 and 501\nobs3 = pe.Obs([samples3], ['ensemble1'], idl=[[2, 9, 28, 29, 501]])\nobs3.details()\n> Result 1.01718064e+00\n> 5 samples in 1 ensemble:\n> \u00b7 Ensemble 'ensemble1' : 5 configurations (irregular range)\n
\n\n
Obs
objects defined on regular and irregular histories of the same ensemble can be combined with each other and the correct error propagation and estimation is automatically taken care of.Warning: Irregular Monte Carlo chains can result in odd patterns in the autocorrelation functions.\nMake sure to check the autocorrelation time with e.g.
\n\npyerrors.obs.Obs.plot_rho
orpyerrors.obs.Obs.plot_tauint
.For the full API see
\n\npyerrors.obs.Obs
.Correlators
\n\nWhen one is not interested in single observables but correlation functions,
\n\npyerrors
offers theCorr
class which simplifies the corresponding error propagation and provides the user with a set of standard methods. In order to initialize aCorr
objects one needs to arrange the data as a list ofObs
\n\n\n\nmy_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3])\nprint(my_corr)\n> x0/a Corr(x0/a)\n> ------------------\n> 0 0.7957(80)\n> 1 0.5156(51)\n> 2 0.3227(33)\n> 3 0.2041(21)\n
In case the correlation functions are not defined on the outermost timeslices, for example because of fixed boundary conditions, a padding can be introduced.
\n\n\n\n\n\nmy_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3], padding=[1, 1])\nprint(my_corr)\n> x0/a Corr(x0/a)\n> ------------------\n> 0\n> 1 0.7957(80)\n> 2 0.5156(51)\n> 3 0.3227(33)\n> 4 0.2041(21)\n> 5\n
The individual entries of a correlator can be accessed via slicing
\n\n\n\n\n\nprint(my_corr[3])\n> 0.3227(33)\n
Error propagation with the
\n\nCorr
class works very similar toObs
objects. Mathematical operations are overloaded andCorr
objects can be computed together with otherCorr
objects,Obs
objects or real numbers and integers.\n\n\n\nmy_new_corr = 0.3 * my_corr[2] * my_corr * my_corr + 12 / my_corr\n
\n\n
pyerrors
provides the user with a set of regularly used methods for the manipulation of correlator objects:\n
\n\n- \n
Corr.gamma_method
applies the gamma method to all entries of the correlator.- \n
Corr.m_eff
to construct effective masses. Various variants for periodic and fixed temporal boundary conditions are available.- \n
Corr.deriv
returns the first derivative of the correlator asCorr
. Different discretizations of the numerical derivative are available.- \n
Corr.second_deriv
returns the second derivative of the correlator asCorr
. Different discretizations of the numerical derivative are available.- \n
Corr.symmetric
symmetrizes parity even correlations functions, assuming periodic boundary conditions.- \n
Corr.anti_symmetric
anti-symmetrizes parity odd correlations functions, assuming periodic boundary conditions.- \n
Corr.T_symmetry
averages a correlator with its time symmetry partner, assuming fixed boundary conditions.- \n
Corr.plateau
extracts a plateau value from the correlator in a given range.- \n
Corr.roll
periodically shifts the correlator.- \n
Corr.reverse
reverses the time ordering of the correlator.- \n
Corr.correlate
constructs a disconnected correlation function from the correlator and anotherCorr
orObs
object.- \n
Corr.reweight
reweights the correlator.\n\n
pyerrors
can also handle matrices of correlation functions and extract energy states from these matrices via a generalized eigenvalue problem (seepyerrors.correlators.Corr.GEVP
).For the full API see
\n\npyerrors.correlators.Corr
.Complex valued observables
\n\n\n\n
pyerrors
can handle complex valued observables via the classpyerrors.obs.CObs
.\nCObs
are initialized with a real and an imaginary part which both can beObs
valued.\n\n\n\nmy_real_part = pe.Obs([samples1], ['ensemble1'])\nmy_imag_part = pe.Obs([samples2], ['ensemble1'])\n\nmy_cobs = pe.CObs(my_real_part, my_imag_part)\nmy_cobs.gamma_method()\nprint(my_cobs)\n> (0.9959(91)+0.659(28)j)\n
Elementary mathematical operations are overloaded and samples are properly propagated as for the
\n\nObs
class.\n\n\n\nmy_derived_cobs = (my_cobs + my_cobs.conjugate()) / np.abs(my_cobs)\nmy_derived_cobs.gamma_method()\nprint(my_derived_cobs)\n> (1.668(23)+0.0j)\n
The
\n\nCovobs
classIn many projects, auxiliary data that is not based on Monte Carlo chains enters. Examples are experimentally determined mesons masses which are used to set the scale or renormalization constants. These numbers come with an error that has to be propagated through the analysis. The
\n\nCovobs
class allows to define such quantities inpyerrors
. Furthermore, external input might consist of correlated quantities. An example are the parameters of an interpolation formula, which are defined via mean values and a covariance matrix between all parameters. The contribution of the interpolation formula to the error of a derived quantity therefore might depend on the complete covariance matrix.This concept is built into the definition of
\n\nCovobs
. Inpyerrors
, external input is defined by $M$ mean values, a $M\\times M$ covariance matrix, where $M=1$ is permissible, and a name that uniquely identifies the covariance matrix. Below, we define the pion mass, based on its mean value and error, 134.9768(5). Note, that the square of the error enterscov_Obs
, since the second argument of this function is the covariance matrix of theCovobs
.\n\n\n\nimport pyerrors.obs as pe\n\nmpi = pe.cov_Obs(134.9768, 0.0005**2, 'pi^0 mass')\nmpi.gamma_method()\nmpi.details()\n> Result 1.34976800e+02 +/- 5.00000000e-04 +/- 0.00000000e+00 (0.000%)\n> pi^0 mass 5.00000000e-04\n> 0 samples in 1 ensemble:\n> \u00b7 Covobs 'pi^0 mass'\n
The resulting object
\n\nmpi
is anObs
that contains aCovobs
. In the following, it may be handled as any otherObs
. The contribution of the covariance matrix to the error of anObs
is determined from the $M \\times M$ covariance matrix $\\Sigma$ and the gradient of theObs
with respect to the external quantities, which is the $1\\times M$ Jacobian matrix $J$, via\n$$s = \\sqrt{J^T \\Sigma J}\\,,$$\nwhere the Jacobian is computed for each derived quantity via automatic differentiation.Correlated auxiliary data is defined similarly to above, e.g., via
\n\n\n\n\n\nRAP = pe.cov_Obs([16.7457, -19.0475], [[3.49591, -6.07560], [-6.07560, 10.5834]], 'R_AP, 1906.03445, (5.3a)')\nprint(RAP)\n> [Obs[16.7(1.9)], Obs[-19.0(3.3)]]\n
where
\n\nRAP
now is a list of twoObs
that contains the two correlated parameters.Since the gradient of a derived observable with respect to an external covariance matrix is propagated through the entire analysis, the
\n\nCovobs
class allows to quote the derivative of a result with respect to the external quantities. If these derivatives are published together with the result, small shifts in the definition of external quantities, e.g., the definition of the physical point, can be performed a posteriori based on the published information. This may help to compare results of different groups. The gradient of anObs
o
with respect to a covariance matrix with the identifying stringk
may be accessed via\n\n\n\no.covobs[k].grad\n
Error propagation in iterative algorithms
\n\n\n\n
pyerrors
supports exact linear error propagation for iterative algorithms like various variants of non-linear least squares fits or root finding. The derivatives required for the error propagation are calculated as described in arXiv:1809.01289.Least squares fits
\n\nStandard non-linear least square fits with errors on the dependent but not the independent variables can be performed with
\n\npyerrors.fits.least_squares
. As default solver the Levenberg-Marquardt algorithm implemented in scipy is used.Fit functions have to be of the following form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[1] * anp.exp(-a[0] * x)\n
It is important that numerical functions refer to
\n\nautograd.numpy
instead ofnumpy
for the automatic differentiation in iterative algorithms to work properly.Fits can then be performed via
\n\n\n\n\n\nfit_result = pe.fits.least_squares(x, y, func)\nprint("\\n", fit_result)\n> Fit with 2 parameters\n> Method: Levenberg-Marquardt\n> `ftol` termination condition is satisfied.\n> chisquare/d.o.f.: 0.9593035785160936\n\n> Goodness of fit:\n> \u03c7\u00b2/d.o.f. = 0.959304\n> p-value = 0.5673\n> Fit parameters:\n> 0 0.0548(28)\n> 1 1.933(64)\n
where x is a
\n\nlist
ornumpy.array
offloats
and y is alist
ornumpy.array
ofObs
.Data stored in
\n\nCorr
objects can be fitted directly using theCorr.fit
method.\n\n\n\nmy_corr = pe.Corr(y)\nfit_result = my_corr.fit(func, fitrange=[12, 25])\n
this can simplify working with absolute fit ranges and takes care of gaps in the data automatically.
\n\nFor fit functions with multiple independent variables the fit function can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
\n\n
pyerrors
also supports correlated fits which can be triggered via the parametercorrelated_fit=True
.\nDetails about how the required covariance matrix is estimated can be found inpyerrors.obs.covariance
.Direct visualizations of the performed fits can be triggered via
\n\nresplot=True
orqqplot=True
. For all available options seepyerrors.fits.least_squares
.Total least squares fits
\n\n\n\n
pyerrors
can also fit data with errors on both the dependent and independent variables using the total least squares method also referred to orthogonal distance regression as implemented in scipy, seepyerrors.fits.least_squares
. The syntax is identical to the standard least squares case, the only difference being thatx
also has to be alist
ornumpy.array
ofObs
.For the full API see
\n\npyerrors.fits
for fits andpyerrors.roots
for finding roots of functions.Matrix operations
\n\n\n\n
pyerrors
provides wrappers forObs
- andCObs
-valued matrix operations based onnumpy.linalg
. The supported functions include:\n
\n\n- \n
inv
for the matrix inverse.- \n
cholseky
for the Cholesky decomposition.- \n
det
for the matrix determinant.- \n
eigh
for eigenvalues and eigenvectors of hermitean matrices.- \n
eig
for eigenvalues of general matrices.- \n
pinv
for the Moore-Penrose pseudoinverse.- \n
svd
for the singular-value-decomposition.For the full API see
\n\npyerrors.linalg
.Export data
\n\nThe preferred exported file format within
\n\npyerrors
is json.gz. Files written to this format are valid JSON files that have been compressed using gzip. The structure of the content is inspired by the dobs format of the ALPHA collaboration. The aim of the format is to facilitate the storage of data in a self-contained way such that, even years after the creation of the file, it is possible to extract all necessary information:\n
\n\n- What observables are stored? Possibly: How exactly are they defined.
\n- How does each single ensemble or external quantity contribute to the error of the observable?
\n- Who did write the file when and on which machine?
\nThis can be achieved by storing all information in one single file. The export routines of
\n\npyerrors
are written such that as much information as possible is written automatically as described in the following example\n\n\n\nmy_obs = pe.Obs([samples], ["test_ensemble"])\nmy_obs.tag = "My observable"\n\npe.input.json.dump_to_json(my_obs, "test_output_file", description="This file contains a test observable")\n# For a single observable one can equivalently use the class method dump\nmy_obs.dump("test_output_file", description="This file contains a test observable")\n\ncheck = pe.input.json.load_json("test_output_file")\n\nprint(my_obs == check)\n> True\n
The format also allows to directly write out the content of
\n\nCorr
objects or lists and arrays ofObs
objects by passing the desired data topyerrors.input.json.dump_to_json
.json.gz format specification
\n\nThe first entries of the file provide optional auxiliary information:
\n\n\n
\n\n- \n
program
is a string that indicates which program was used to write the file.- \n
version
is a string that specifies the version of the format.- \n
who
is a string that specifies the user name of the creator of the file.- \n
date
is a string and contains the creation date of the file.- \n
host
is a string and contains the hostname of the machine where the file has been written.- \n
description
contains information on the content of the file. This field is not filled automatically inpyerrors
. The user is advised to provide as detailed information as possible in this field. Examples are: Input files of measurements or simulations, LaTeX formulae or references to publications to specify how the observables have been computed, details on the analysis strategy, ... This field may be any valid JSON type. Strings, arrays or objects (equivalent to dicts in python) are well suited to provide information.The only necessary entry of the file is the field\n-
\n\nobsdata
, an array that contains the actual data.Each entry of the array belongs to a single structure of observables. Currently, these structures can be either of
\n\nObs
,list
,numpy.ndarray
,Corr
. AllObs
inside a structure (with dimension > 0) have to be defined on the same set of configurations. Different structures, that are represented by entries of the arrayobsdata
, are treated independently. Each entry of the arrayobsdata
has the following required entries:\n
\n\n- \n
type
is a string that specifies the type of the structure. This allows to parse the content to the correct form after reading the file. It is always possible to interpret the content as list of Obs.- \n
value
is an array that contains the mean values of the Obs inside the structure.\nThe following entries are optional:- \n
layout
is a string that specifies the layout of multi-dimensional structures. Examples are \"2, 2\" for a 2x2 dimensional matrix or \"64, 4, 4\" for a Corr with $T=64$ and 4x4 matrices on each time slices. \"1\" denotes a single Obs. Multi-dimensional structures are stored in row-major format (see below).- \n
tag
is any JSON type. It contains additional information concerning the structure. Thetag
of anObs
inpyerrors
is written here.- \n
reweighted
is a Bool that may be used to specify, whether theObs
in the structure have been reweighted.- \n
data
is an array that contains the data from MC chains. We will define it below.- \n
cdata
is an array that contains the data from external quantities with an error (Covobs
inpyerrors
). We will define it below.The array
\n\ndata
contains the data from MC chains. Each entry of the array corresponds to one ensemble and contains:\n
\n\n- \n
id
, a string that contains the name of the ensemble- \n
replica
, an array that contains an entry per replica of the ensemble.Each entry of
\n\nreplica
contains\nname
, a string that contains the name of the replica\ndeltas
, an array that contains the actual data.Each entry in
\n\ndeltas
corresponds to one configuration of the replica and has $1+N$ many entries. The first entry is an integer that specifies the configuration number that, together with ensemble and replica name, may be used to uniquely identify the configuration on which the data has been obtained. The following N entries specify the deltas, i.e., the deviation of the observable from the mean value on this configuration, of eachObs
inside the structure. Multi-dimensional structures are stored in a row-major format. For primary observables, such as correlation functions, $value + delta_i$ matches the primary data obtained on the configuration.The array
\n\ncdata
contains information about the contribution of auxiliary observables, represented byCovobs
inpyerrors
, to the total error of the observables. Each entry of the array belongs to one auxiliary covariance matrix and contains:\n
\n\n- \n
id
, a string that identifies the covariance matrix- \n
layout
, a string that defines the dimensions of the $M\\times M$ covariance matrix (has to be \"M, M\" or \"1\").- \n
cov
, an array that contains the $M\\times M$ many entries of the covariance matrix, stored in row-major format.- \n
grad
, an array that contains N entries, one for eachObs
inside the structure. Each entry itself is an array, that contains the M gradients of the Nth observable with respect to the quantity that corresponds to the Mth diagonal entry of the covariance matrix.A JSON schema that may be used to verify the correctness of a file with respect to the format definition is stored in ./examples/json_schema.json. The schema is a self-descriptive format definition and contains an exemplary file.
\n\nJulia I/O routines for the json.gz format, compatible with ADerrors.jl, can be found here.
\n"}, "pyerrors.correlators": {"fullname": "pyerrors.correlators", "modulename": "pyerrors.correlators", "kind": "module", "doc": "\n"}, "pyerrors.correlators.Corr": {"fullname": "pyerrors.correlators.Corr", "modulename": "pyerrors.correlators", "qualname": "Corr", "kind": "class", "doc": "The class for a correlator (time dependent sequence of pe.Obs).
\n\nEverything, this class does, can be achieved using lists or arrays of Obs.\nBut it is simply more convenient to have a dedicated object for correlators.\nOne often wants to add or multiply correlators of the same length at every timeslice and it is inconvenient\nto iterate over all timeslices for every operation. This is especially true, when dealing with matrices.
\n\nThe correlator can have two types of content: An Obs at every timeslice OR a GEVP\nmatrix at every timeslice. Other dependency (eg. spatial) are not supported.
\n"}, "pyerrors.correlators.Corr.__init__": {"fullname": "pyerrors.correlators.Corr.__init__", "modulename": "pyerrors.correlators", "qualname": "Corr.__init__", "kind": "function", "doc": "Initialize a Corr object.
\n\nParameters
\n\n\n
\n", "signature": "(data_input, padding=[0, 0], prange=None)"}, "pyerrors.correlators.Corr.gamma_method": {"fullname": "pyerrors.correlators.Corr.gamma_method", "modulename": "pyerrors.correlators", "qualname": "Corr.gamma_method", "kind": "function", "doc": "- data_input (list or array):\nlist of Obs or list of arrays of Obs or array of Corrs
\n- padding (list, optional):\nList with two entries where the first labels the padding\nat the front of the correlator and the second the padding\nat the back.
\n- prange (list, optional):\nList containing the first and last timeslice of the plateau\nregion indentified for this correlator.
\nApply the gamma method to the content of the Corr.
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.gm": {"fullname": "pyerrors.correlators.Corr.gm", "modulename": "pyerrors.correlators", "qualname": "Corr.gm", "kind": "function", "doc": "Apply the gamma method to the content of the Corr.
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.projected": {"fullname": "pyerrors.correlators.Corr.projected", "modulename": "pyerrors.correlators", "qualname": "Corr.projected", "kind": "function", "doc": "We need to project the Correlator with a Vector to get a single value at each timeslice.
\n\nThe method can use one or two vectors.\nIf two are specified it returns v1@G@v2 (the order might be very important.)\nBy default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to
\n", "signature": "(self, vector_l=None, vector_r=None, normalize=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.item": {"fullname": "pyerrors.correlators.Corr.item", "modulename": "pyerrors.correlators", "qualname": "Corr.item", "kind": "function", "doc": "Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice.
\n\nParameters
\n\n\n
\n", "signature": "(self, i, j):", "funcdef": "def"}, "pyerrors.correlators.Corr.plottable": {"fullname": "pyerrors.correlators.Corr.plottable", "modulename": "pyerrors.correlators", "qualname": "Corr.plottable", "kind": "function", "doc": "- i (int):\nFirst index to be picked.
\n- j (int):\nSecond index to be picked.
\nOutputs the correlator in a plotable format.
\n\nOutputs three lists containing the timeslice index, the value on each\ntimeslice and the error on each timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.symmetric": {"fullname": "pyerrors.correlators.Corr.symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.symmetric", "kind": "function", "doc": "Symmetrize the correlator around x0=0.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.anti_symmetric": {"fullname": "pyerrors.correlators.Corr.anti_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.anti_symmetric", "kind": "function", "doc": "Anti-symmetrize the correlator around x0=0.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.is_matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.is_matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.is_matrix_symmetric", "kind": "function", "doc": "Checks whether a correlator matrices is symmetric on every timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.matrix_symmetric", "kind": "function", "doc": "Symmetrizes the correlator matrices on every timeslice.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.GEVP": {"fullname": "pyerrors.correlators.Corr.GEVP", "modulename": "pyerrors.correlators", "qualname": "Corr.GEVP", "kind": "function", "doc": "Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors.
\n\nThe eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the\nlargest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing
\n\n\n\n\n\nC.GEVP(t0=2)[0] # Ground state vector(s)\nC.GEVP(t0=2)[:3] # Vectors for the lowest three states\n
Parameters
\n\n\n
\n\n- t0 (int):\nThe time t0 for the right hand side of the GEVP according to $G(t)v_i=\\lambda_i G(t_0)v_i$
\n- ts (int):\nfixed time $G(t_s)v_i=\\lambda_i G(t_0)v_i$ if sort=None.\nIf sort=\"Eigenvector\" it gives a reference point for the sorting method.
\n- sort (string):\nIf this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned.\n
\n\n
- \"Eigenvalue\": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice.
\n- \"Eigenvector\": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state.\nThe reference state is identified by its eigenvalue at $t=t_s$.
\nOther Parameters
\n\n\n
\n", "signature": "(self, t0, ts=None, sort='Eigenvalue', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.Eigenvalue": {"fullname": "pyerrors.correlators.Corr.Eigenvalue", "modulename": "pyerrors.correlators", "qualname": "Corr.Eigenvalue", "kind": "function", "doc": "- state (int):\nReturns only the vector(s) for a specified state. The lowest state is zero.
\nDetermines the eigenvalue of the GEVP by solving and projecting the correlator
\n\nParameters
\n\n\n
\n", "signature": "(self, t0, ts=None, state=0, sort='Eigenvalue'):", "funcdef": "def"}, "pyerrors.correlators.Corr.Hankel": {"fullname": "pyerrors.correlators.Corr.Hankel", "modulename": "pyerrors.correlators", "qualname": "Corr.Hankel", "kind": "function", "doc": "- state (int):\nThe state one is interested in ordered by energy. The lowest state is zero.
\n- All other parameters are identical to the ones of Corr.GEVP.
\nConstructs an NxN Hankel matrix
\n\nC(t) c(t+1) ... c(t+n-1)\nC(t+1) c(t+2) ... c(t+n)\n.................\nC(t+(n-1)) c(t+n) ... c(t+2(n-1))
\n\nParameters
\n\n\n
\n", "signature": "(self, N, periodic=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.roll": {"fullname": "pyerrors.correlators.Corr.roll", "modulename": "pyerrors.correlators", "qualname": "Corr.roll", "kind": "function", "doc": "- N (int):\nDimension of the Hankel matrix
\n- periodic (bool, optional):\ndetermines whether the matrix is extended periodically
\nPeriodically shift the correlator by dt timeslices
\n\nParameters
\n\n\n
\n", "signature": "(self, dt):", "funcdef": "def"}, "pyerrors.correlators.Corr.reverse": {"fullname": "pyerrors.correlators.Corr.reverse", "modulename": "pyerrors.correlators", "qualname": "Corr.reverse", "kind": "function", "doc": "- dt (int):\nnumber of timeslices
\nReverse the time ordering of the Corr
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.thin": {"fullname": "pyerrors.correlators.Corr.thin", "modulename": "pyerrors.correlators", "qualname": "Corr.thin", "kind": "function", "doc": "Thin out a correlator to suppress correlations
\n\nParameters
\n\n\n
\n", "signature": "(self, spacing=2, offset=0):", "funcdef": "def"}, "pyerrors.correlators.Corr.correlate": {"fullname": "pyerrors.correlators.Corr.correlate", "modulename": "pyerrors.correlators", "qualname": "Corr.correlate", "kind": "function", "doc": "- spacing (int):\nKeep only every 'spacing'th entry of the correlator
\n- offset (int):\nOffset the equal spacing
\nCorrelate the correlator with another correlator or Obs
\n\nParameters
\n\n\n
\n", "signature": "(self, partner):", "funcdef": "def"}, "pyerrors.correlators.Corr.reweight": {"fullname": "pyerrors.correlators.Corr.reweight", "modulename": "pyerrors.correlators", "qualname": "Corr.reweight", "kind": "function", "doc": "- partner (Obs or Corr):\npartner to correlate the correlator with.\nCan either be an Obs which is correlated with all entries of the\ncorrelator or a Corr of same length.
\nReweight the correlator.
\n\nParameters
\n\n\n
\n", "signature": "(self, weight, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.T_symmetry": {"fullname": "pyerrors.correlators.Corr.T_symmetry", "modulename": "pyerrors.correlators", "qualname": "Corr.T_symmetry", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl.
\nReturn the time symmetry average of the correlator and its partner
\n\nParameters
\n\n\n
\n", "signature": "(self, partner, parity=1):", "funcdef": "def"}, "pyerrors.correlators.Corr.deriv": {"fullname": "pyerrors.correlators.Corr.deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.deriv", "kind": "function", "doc": "- partner (Corr):\nTime symmetry partner of the Corr
\n- partity (int):\nParity quantum number of the correlator, can be +1 or -1
\nReturn the first derivative of the correlator with respect to x0.
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.second_deriv": {"fullname": "pyerrors.correlators.Corr.second_deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.second_deriv", "kind": "function", "doc": "- variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, forward, backward, improved, log, default: symmetric
\nReturn the second derivative of the correlator with respect to x0.
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.m_eff": {"fullname": "pyerrors.correlators.Corr.m_eff", "modulename": "pyerrors.correlators", "qualname": "Corr.m_eff", "kind": "function", "doc": "- variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, improved, log, default: symmetric
\nReturns the effective mass of the correlator as correlator object
\n\nParameters
\n\n\n
\n", "signature": "(self, variant='log', guess=1.0):", "funcdef": "def"}, "pyerrors.correlators.Corr.fit": {"fullname": "pyerrors.correlators.Corr.fit", "modulename": "pyerrors.correlators", "qualname": "Corr.fit", "kind": "function", "doc": "- variant (str):\nlog : uses the standard effective mass log(C(t) / C(t+1))\ncosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m.\nsinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m.\nSee, e.g., arXiv:1205.5380\narccosh : Uses the explicit form of the symmetrized correlator (not recommended)\nlogsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2
\n- guess (float):\nguess for the root finder, only relevant for the root variant
\nFits function to the data
\n\nParameters
\n\n\n
\n", "signature": "(self, function, fitrange=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.plateau": {"fullname": "pyerrors.correlators.Corr.plateau", "modulename": "pyerrors.correlators", "qualname": "Corr.plateau", "kind": "function", "doc": "- function (obj):\nfunction to fit to the data. See fits.least_squares for details.
\n- fitrange (list):\nTwo element list containing the timeslices on which the fit is supposed to start and stop.\nCaution: This range is inclusive as opposed to standard python indexing.\n
\nfitrange=[4, 6]
corresponds to the three entries 4, 5 and 6.\nIf not specified, self.prange or all timeslices are used.- silent (bool):\nDecides whether output is printed to the standard output.
\nExtract a plateau value from a Corr object
\n\nParameters
\n\n\n
\n", "signature": "(self, plateau_range=None, method='fit', auto_gamma=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.set_prange": {"fullname": "pyerrors.correlators.Corr.set_prange", "modulename": "pyerrors.correlators", "qualname": "Corr.set_prange", "kind": "function", "doc": "- plateau_range (list):\nlist with two entries, indicating the first and the last timeslice\nof the plateau region.
\n- method (str):\nmethod to extract the plateau.\n 'fit' fits a constant to the plateau region\n 'avg', 'average' or 'mean' just average over the given timeslices.
\n- auto_gamma (bool):\napply gamma_method with default parameters to the Corr. Defaults to None
\nSets the attribute prange of the Corr object.
\n", "signature": "(self, prange):", "funcdef": "def"}, "pyerrors.correlators.Corr.show": {"fullname": "pyerrors.correlators.Corr.show", "modulename": "pyerrors.correlators", "qualname": "Corr.show", "kind": "function", "doc": "Plots the correlator using the tag of the correlator as label if available.
\n\nParameters
\n\n\n
\n", "signature": "(\tself,\tx_range=None,\tcomp=None,\ty_range=None,\tlogscale=False,\tplateau=None,\tfit_res=None,\tylabel=None,\tsave=None,\tauto_gamma=False,\thide_sigma=None,\treferences=None,\ttitle=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.spaghetti_plot": {"fullname": "pyerrors.correlators.Corr.spaghetti_plot", "modulename": "pyerrors.correlators", "qualname": "Corr.spaghetti_plot", "kind": "function", "doc": "- x_range (list):\nlist of two values, determining the range of the x-axis e.g. [4, 8].
\n- comp (Corr or list of Corr):\nCorrelator or list of correlators which are plotted for comparison.\nThe tags of these correlators are used as labels if available.
\n- logscale (bool):\nSets y-axis to logscale.
\n- plateau (Obs):\nPlateau value to be visualized in the figure.
\n- fit_res (Fit_result):\nFit_result object to be visualized.
\n- ylabel (str):\nLabel for the y-axis.
\n- save (str):\npath to file in which the figure should be saved.
\n- auto_gamma (bool):\nApply the gamma method with standard parameters to all correlators and plateau values before plotting.
\n- hide_sigma (float):\nHides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors.
\n- references (list):\nList of floating point values that are displayed as horizontal lines for reference.
\n- title (string):\nOptional title of the figure.
\nProduces a spaghetti plot of the correlator suited to monitor exceptional configurations.
\n\nParameters
\n\n\n
\n", "signature": "(self, logscale=True):", "funcdef": "def"}, "pyerrors.correlators.Corr.dump": {"fullname": "pyerrors.correlators.Corr.dump", "modulename": "pyerrors.correlators", "qualname": "Corr.dump", "kind": "function", "doc": "- logscale (bool):\nDetermines whether the scale of the y-axis is logarithmic or standard.
\nDumps the Corr into a file of chosen type
\n\nParameters
\n\n\n
\n", "signature": "(self, filename, datatype='json.gz', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.print": {"fullname": "pyerrors.correlators.Corr.print", "modulename": "pyerrors.correlators", "qualname": "Corr.print", "kind": "function", "doc": "\n", "signature": "(self, print_range=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.sqrt": {"fullname": "pyerrors.correlators.Corr.sqrt", "modulename": "pyerrors.correlators", "qualname": "Corr.sqrt", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.log": {"fullname": "pyerrors.correlators.Corr.log", "modulename": "pyerrors.correlators", "qualname": "Corr.log", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.exp": {"fullname": "pyerrors.correlators.Corr.exp", "modulename": "pyerrors.correlators", "qualname": "Corr.exp", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sin": {"fullname": "pyerrors.correlators.Corr.sin", "modulename": "pyerrors.correlators", "qualname": "Corr.sin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cos": {"fullname": "pyerrors.correlators.Corr.cos", "modulename": "pyerrors.correlators", "qualname": "Corr.cos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tan": {"fullname": "pyerrors.correlators.Corr.tan", "modulename": "pyerrors.correlators", "qualname": "Corr.tan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sinh": {"fullname": "pyerrors.correlators.Corr.sinh", "modulename": "pyerrors.correlators", "qualname": "Corr.sinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cosh": {"fullname": "pyerrors.correlators.Corr.cosh", "modulename": "pyerrors.correlators", "qualname": "Corr.cosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tanh": {"fullname": "pyerrors.correlators.Corr.tanh", "modulename": "pyerrors.correlators", "qualname": "Corr.tanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsin": {"fullname": "pyerrors.correlators.Corr.arcsin", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccos": {"fullname": "pyerrors.correlators.Corr.arccos", "modulename": "pyerrors.correlators", "qualname": "Corr.arccos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctan": {"fullname": "pyerrors.correlators.Corr.arctan", "modulename": "pyerrors.correlators", "qualname": "Corr.arctan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsinh": {"fullname": "pyerrors.correlators.Corr.arcsinh", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccosh": {"fullname": "pyerrors.correlators.Corr.arccosh", "modulename": "pyerrors.correlators", "qualname": "Corr.arccosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctanh": {"fullname": "pyerrors.correlators.Corr.arctanh", "modulename": "pyerrors.correlators", "qualname": "Corr.arctanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.prune": {"fullname": "pyerrors.correlators.Corr.prune", "modulename": "pyerrors.correlators", "qualname": "Corr.prune", "kind": "function", "doc": "- filename (str):\nName of the file to be saved.
\n- datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
\n- path (str):\nspecifies a custom path for the file (default '.')
\nProject large correlation matrix to lowest states
\n\nThis method can be used to reduce the size of an (N x N) correlation matrix\nto (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise\nis still small.
\n\nParameters
\n\n\n
\n\n- Ntrunc (int):\nRank of the target matrix.
\n- tproj (int):\nTime where the eigenvectors are evaluated, corresponds to ts in the GEVP method.\nThe default value is 3.
\n- t0proj (int):\nTime where the correlation matrix is inverted. Choosing t0proj=1 is strongly\ndiscouraged for O(a) improved theories, since the correctness of the procedure\ncannot be granted in this case. The default value is 2.
\n- basematrix (Corr):\nCorrelation matrix that is used to determine the eigenvectors of the\nlowest states based on a GEVP. basematrix is taken to be the Corr itself if\nis is not specified.
\nNotes
\n\nWe have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving\nthe GEVP $$C(t) v_n(t, t_0) = \\lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \\equiv t_\\mathrm{proj}$\nand $t_0 \\equiv t_{0, \\mathrm{proj}}$. The target matrix is projected onto the subspace of the\nresulting eigenvectors $v_n, n=1,\\dots,N_\\mathrm{trunc}$ via\n$$G^\\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large\ncorrelation matrix and to remove some noise that is added by irrelevant operators.\nThis may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated\nbound $t_0 \\leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$.
\n", "signature": "(self, Ntrunc, tproj=3, t0proj=2, basematrix=None):", "funcdef": "def"}, "pyerrors.covobs": {"fullname": "pyerrors.covobs", "modulename": "pyerrors.covobs", "kind": "module", "doc": "\n"}, "pyerrors.covobs.Covobs": {"fullname": "pyerrors.covobs.Covobs", "modulename": "pyerrors.covobs", "qualname": "Covobs", "kind": "class", "doc": "\n"}, "pyerrors.covobs.Covobs.__init__": {"fullname": "pyerrors.covobs.Covobs.__init__", "modulename": "pyerrors.covobs", "qualname": "Covobs.__init__", "kind": "function", "doc": "Initialize Covobs object.
\n\nParameters
\n\n\n
\n", "signature": "(mean, cov, name, pos=None, grad=None)"}, "pyerrors.covobs.Covobs.errsq": {"fullname": "pyerrors.covobs.Covobs.errsq", "modulename": "pyerrors.covobs", "qualname": "Covobs.errsq", "kind": "function", "doc": "- mean (float):\nMean value of the new Obs
\n- cov (list or array):\n2d Covariance matrix or 1d diagonal entries
\n- name (str):\nidentifier for the covariance matrix
\n- pos (int):\nPosition of the variance belonging to mean in cov.\nIs taken to be 1 if cov is 0-dimensional
\n- grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
\nReturn the variance (= square of the error) of the Covobs
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.dirac": {"fullname": "pyerrors.dirac", "modulename": "pyerrors.dirac", "kind": "module", "doc": "\n"}, "pyerrors.dirac.epsilon_tensor": {"fullname": "pyerrors.dirac.epsilon_tensor", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor", "kind": "function", "doc": "Rank-3 epsilon tensor
\n\nBased on https://codegolf.stackexchange.com/a/160375
\n", "signature": "(i, j, k):", "funcdef": "def"}, "pyerrors.dirac.epsilon_tensor_rank4": {"fullname": "pyerrors.dirac.epsilon_tensor_rank4", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor_rank4", "kind": "function", "doc": "Rank-4 epsilon tensor
\n\nExtension of https://codegolf.stackexchange.com/a/160375
\n", "signature": "(i, j, k, o):", "funcdef": "def"}, "pyerrors.dirac.Grid_gamma": {"fullname": "pyerrors.dirac.Grid_gamma", "modulename": "pyerrors.dirac", "qualname": "Grid_gamma", "kind": "function", "doc": "Returns gamma matrix in Grid labeling.
\n", "signature": "(gamma_tag):", "funcdef": "def"}, "pyerrors.fits": {"fullname": "pyerrors.fits", "modulename": "pyerrors.fits", "kind": "module", "doc": "\n"}, "pyerrors.fits.Fit_result": {"fullname": "pyerrors.fits.Fit_result", "modulename": "pyerrors.fits", "qualname": "Fit_result", "kind": "class", "doc": "Represents fit results.
\n\nAttributes
\n\n\n
\n", "bases": "collections.abc.Sequence"}, "pyerrors.fits.Fit_result.__init__": {"fullname": "pyerrors.fits.Fit_result.__init__", "modulename": "pyerrors.fits", "qualname": "Fit_result.__init__", "kind": "function", "doc": "\n", "signature": "()"}, "pyerrors.fits.Fit_result.gamma_method": {"fullname": "pyerrors.fits.Fit_result.gamma_method", "modulename": "pyerrors.fits", "qualname": "Fit_result.gamma_method", "kind": "function", "doc": "- fit_parameters (list):\nresults for the individual fit parameters,\nalso accessible via indices.
\n- chisquare_by_dof (float):\nreduced chisquare.
\n- p_value (float):\np-value of the fit
\n- t2_p_value (float):\nHotelling t-squared p-value for correlated fits.
\nApply the gamma method to all fit parameters
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.Fit_result.gm": {"fullname": "pyerrors.fits.Fit_result.gm", "modulename": "pyerrors.fits", "qualname": "Fit_result.gm", "kind": "function", "doc": "Apply the gamma method to all fit parameters
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.least_squares": {"fullname": "pyerrors.fits.least_squares", "modulename": "pyerrors.fits", "qualname": "least_squares", "kind": "function", "doc": "Performs a non-linear fit to y = func(x).
\n\nParameters
\n\n\n
\n", "signature": "(x, y, func, priors=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.total_least_squares": {"fullname": "pyerrors.fits.total_least_squares", "modulename": "pyerrors.fits", "qualname": "total_least_squares", "kind": "function", "doc": "- x (list):\nlist of floats.
\n- y (list):\nlist of Obs.
\n- \n
func (object):\nfit function, has to be of the form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
For multiple x values func can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.
- priors (list, optional):\npriors has to be a list with an entry for every parameter in the fit. The entries can either be\nObs (e.g. results from a previous fit) or strings containing a value and an error formatted like\n0.548(23), 500(40) or 0.5(0.4)
\n- silent (bool, optional):\nIf true all output to the console is omitted (default False).
\n- initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for\nnon-linear fits with many parameters. In case of correlated fits the guess is used to perform\nan uncorrelated fit which then serves as guess for the correlated fit.
\n- method (str, optional):\ncan be used to choose an alternative method for the minimization of chisquare.\nThe possible methods are the ones which can be used for scipy.optimize.minimize and\nmigrad of iminuit. If no method is specified, Levenberg-Marquard is used.\nReliable alternatives are migrad, Powell and Nelder-Mead.
\n- correlated_fit (bool):\nIf True, use the full inverse covariance matrix in the definition of the chisquare cost function.\nFor details about how the covariance matrix is estimated see
\npyerrors.obs.covariance
.\nIn practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix).\nThis procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning).\nAt the moment this option only works forprior==None
and when nomethod
is given.- expected_chisquare (bool):\nIf True estimates the expected chisquare which is\ncorrected by effects caused by correlated input data (default False).
\n- resplot (bool):\nIf True, a plot which displays fit, data and residuals is generated (default False).
\n- qqplot (bool):\nIf True, a quantile-quantile plot of the fit result is generated (default False).
\n- num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
\nPerforms a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters.
\n\nParameters
\n\n\n
\n\n- x (list):\nlist of Obs, or a tuple of lists of Obs
\n- y (list):\nlist of Obs. The dvalues of the Obs are used as x- and yerror for the fit.
\n- \n
func (object):\nfunc has to be of the form
\n\n\n\n\n\nimport autograd.numpy as anp\n\ndef func(a, x):\n return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
For multiple x values func can be of the form
\n\n\n\n\n\ndef func(a, x):\n (x1, x2) = x\n return a[0] * x1 ** 2 + a[1] * x2\n
It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.
- silent (bool, optional):\nIf true all output to the console is omitted (default False).
\n- initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for non-linear\nfits with many parameters.
\n- expected_chisquare (bool):\nIf true prints the expected chisquare which is\ncorrected by effects caused by correlated input data.\nThis can take a while as the full correlation matrix\nhas to be calculated (default False).
\n- num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
\nNotes
\n\nBased on the orthogonal distance regression module of scipy
\n", "signature": "(x, y, func, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.fit_lin": {"fullname": "pyerrors.fits.fit_lin", "modulename": "pyerrors.fits", "qualname": "fit_lin", "kind": "function", "doc": "Performs a linear fit to y = n + m * x and returns two Obs n, m.
\n\nParameters
\n\n\n
\n", "signature": "(x, y, **kwargs):", "funcdef": "def"}, "pyerrors.fits.qqplot": {"fullname": "pyerrors.fits.qqplot", "modulename": "pyerrors.fits", "qualname": "qqplot", "kind": "function", "doc": "- x (list):\nCan either be a list of floats in which case no xerror is assumed, or\na list of Obs, where the dvalues of the Obs are used as xerror for the fit.
\n- y (list):\nList of Obs, the dvalues of the Obs are used as yerror for the fit.
\nGenerates a quantile-quantile plot of the fit result which can be used to\ncheck if the residuals of the fit are gaussian distributed.
\n", "signature": "(x, o_y, func, p):", "funcdef": "def"}, "pyerrors.fits.residual_plot": {"fullname": "pyerrors.fits.residual_plot", "modulename": "pyerrors.fits", "qualname": "residual_plot", "kind": "function", "doc": "Generates a plot which compares the fit to the data and displays the corresponding residuals
\n", "signature": "(x, y, func, fit_res):", "funcdef": "def"}, "pyerrors.fits.error_band": {"fullname": "pyerrors.fits.error_band", "modulename": "pyerrors.fits", "qualname": "error_band", "kind": "function", "doc": "Returns the error band for an array of sample values x, for given fit function func with optimized parameters beta.
\n", "signature": "(x, func, beta):", "funcdef": "def"}, "pyerrors.fits.ks_test": {"fullname": "pyerrors.fits.ks_test", "modulename": "pyerrors.fits", "qualname": "ks_test", "kind": "function", "doc": "Performs a Kolmogorov\u2013Smirnov test for the p-values of all fit object.
\n\nParameters
\n\n\n
\n", "signature": "(objects=None):", "funcdef": "def"}, "pyerrors.input": {"fullname": "pyerrors.input", "modulename": "pyerrors.input", "kind": "module", "doc": "- objects (list):\nList of fit results to include in the analysis (optional).
\n\n\n
pyerrors
includes aninput
submodule in which input routines and parsers for the output of various numerical programs are contained.Jackknife samples
\n\nFor comparison with other analysis workflows
\n"}, "pyerrors.input.bdio": {"fullname": "pyerrors.input.bdio", "modulename": "pyerrors.input.bdio", "kind": "module", "doc": "\n"}, "pyerrors.input.bdio.read_ADerrors": {"fullname": "pyerrors.input.bdio.read_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "read_ADerrors", "kind": "function", "doc": "pyerrors
can also generate jackknife samples from anObs
object or import jackknife samples into anObs
object.\nSeepyerrors.obs.Obs.export_jackknife
andpyerrors.obs.import_jackknife
for details.Extract generic MCMC data from a bdio file
\n\nread_ADerrors requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.write_ADerrors": {"fullname": "pyerrors.input.bdio.write_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "write_ADerrors", "kind": "function", "doc": "- file_path -- path to the bdio file
\n- bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
\nWrite Obs to a bdio file according to ADerrors conventions
\n\nread_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(obs_list, file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_mesons": {"fullname": "pyerrors.input.bdio.read_mesons", "modulename": "pyerrors.input.bdio", "qualname": "read_mesons", "kind": "function", "doc": "- file_path -- path to the bdio file
\n- bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
\nExtract mesons data from a bdio file and return it as a dictionary
\n\nThe dictionary can be accessed with a tuple consisting of (type, source_position, kappa1, kappa2)
\n\nread_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_dSdm": {"fullname": "pyerrors.input.bdio.read_dSdm", "modulename": "pyerrors.input.bdio", "qualname": "read_dSdm", "kind": "function", "doc": "- file_path (str):\npath to the bdio file
\n- bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
\n- start (int):\nThe first configuration to be read (default 1)
\n- stop (int):\nThe last configuration to be read (default None)
\n- step (int):\nFixed step size between two measurements (default 1)
\n- alternative_ensemble_name (str):\nManually overwrite ensemble name
\nExtract dSdm data from a bdio file and return it as a dictionary
\n\nThe dictionary can be accessed with a tuple consisting of (type, kappa)
\n\nread_dSdm requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to
\n\nall: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/
\n\nParameters
\n\n\n
\n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.dobs": {"fullname": "pyerrors.input.dobs", "modulename": "pyerrors.input.dobs", "kind": "module", "doc": "\n"}, "pyerrors.input.dobs.create_pobs_string": {"fullname": "pyerrors.input.dobs.create_pobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_pobs_string", "kind": "function", "doc": "- file_path (str):\npath to the bdio file
\n- bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
\n- start (int):\nThe first configuration to be read (default 1)
\n- stop (int):\nThe last configuration to be read (default None)
\n- step (int):\nFixed step size between two measurements (default 1)
\n- alternative_ensemble_name (str):\nManually overwrite ensemble name
\nExport a list of Obs or structures containing Obs to an xml string\naccording to the Zeuthen pobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(obsl, name, spec='', origin='', symbol=[], enstag=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_pobs": {"fullname": "pyerrors.input.dobs.write_pobs", "modulename": "pyerrors.input.dobs", "qualname": "write_pobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
\nExport a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen pobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tfname,\tname,\tspec='',\torigin='',\tsymbol=[],\tenstag=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_pobs": {"fullname": "pyerrors.input.dobs.read_pobs", "modulename": "pyerrors.input.dobs", "qualname": "read_pobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
\n- fname (str):\nFilename of the output file.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
\n- gz (bool):\nIf True, the output is a gzipped xml. If False, the output is an xml file.
\nImport a list of Obs from an xml.gz file in the Zeuthen pobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(fname, full_output=False, gz=True, separator_insertion=None):", "funcdef": "def"}, "pyerrors.input.dobs.import_dobs_string": {"fullname": "pyerrors.input.dobs.import_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "import_dobs_string", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- separatior_insertion (str or int):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nNone (default): Replica names remain unchanged.
\nImport a list of Obs from a string in the Zeuthen dobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(content, noempty=False, full_output=False, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_dobs": {"fullname": "pyerrors.input.dobs.read_dobs", "modulename": "pyerrors.input.dobs", "qualname": "read_dobs", "kind": "function", "doc": "- content (str):\nXML string containing the data
\n- noemtpy (bool):\nIf True, ensembles with no contribution to the Obs are not included.\nIf False, ensembles are included as written in the file, possibly with vanishing entries.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
\nImport a list of Obs from an xml.gz file in the Zeuthen dobs format.
\n\nTags are not written or recovered automatically.
\n\nParameters
\n\n\n
\n", "signature": "(\tfname,\tnoempty=False,\tfull_output=False,\tgz=True,\tseparator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.create_dobs_string": {"fullname": "pyerrors.input.dobs.create_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_dobs_string", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- noemtpy (bool):\nIf True, ensembles with no contribution to the Obs are not included.\nIf False, ensembles are included as written in the file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes XML file.
\n- separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
\nGenerate the string for the export of a list of Obs or structures containing Obs\nto a .xml.gz file according to the Zeuthen dobs format.
\n\nTags are not written or recovered automatically. The separator |is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_dobs": {"fullname": "pyerrors.input.dobs.write_dobs", "modulename": "pyerrors.input.dobs", "qualname": "write_dobs", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- who (str):\nProvide the name of the person that exports the data.
\n- enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
\nExport a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen dobs format.
\n\nTags are not written or recovered automatically. The separator | is removed from the replica names.
\n\nParameters
\n\n\n
\n", "signature": "(\tobsl,\tfname,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.hadrons": {"fullname": "pyerrors.input.hadrons", "modulename": "pyerrors.input.hadrons", "kind": "module", "doc": "\n"}, "pyerrors.input.hadrons.read_meson_hd5": {"fullname": "pyerrors.input.hadrons.read_meson_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_meson_hd5", "kind": "function", "doc": "- obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
\n- fname (str):\nFilename of the output file.
\n- name (str):\nThe name of the observable.
\n- spec (str):\nOptional string that describes the contents of the file.
\n- origin (str):\nSpecify where the data has its origin.
\n- symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
\n- who (str):\nProvide the name of the person that exports the data.
\n- enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
\n- gz (bool):\nIf True, the output is a gzipped XML. If False, the output is a XML file.
\nRead hadrons meson hdf5 file and extract the meson labeled 'meson'
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_DistillationContraction_hd5": {"fullname": "pyerrors.input.hadrons.read_DistillationContraction_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_DistillationContraction_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- meson (str):\nlabel of the meson to be extracted, standard value meson_0 which\ncorresponds to the pseudoscalar pseudoscalar two-point function.
\n- gammas (tuple of strings):\nInstrad of a meson label one can also provide a tuple of two strings\nindicating the gamma matrices at source and sink.\n(\"Gamma5\", \"Gamma5\") corresponds to the pseudoscalar pseudoscalar\ntwo-point function. The gammas argument dominateds over meson.
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons DistillationContraction hdf5 files in given directory structure
\n\nParameters
\n\n\n
\n", "signature": "(path, ens_id, diagrams=['direct'], idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.Npr_matrix": {"fullname": "pyerrors.input.hadrons.Npr_matrix", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix", "kind": "class", "doc": "- path (str):\npath to the directories to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- diagrams (list):\nList of strings of the diagrams to extract, e.g. [\"direct\", \"box\", \"cross\"].
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nndarray(shape, dtype=float, buffer=None, offset=0,\n strides=None, order=None)
\n\nAn array object represents a multidimensional, homogeneous array\nof fixed-size items. An associated data-type object describes the\nformat of each element in the array (its byte-order, how many bytes it\noccupies in memory, whether it is an integer, a floating point number,\nor something else, etc.)
\n\nArrays should be constructed using
\n\narray
,zeros
orempty
(refer\nto the See Also section below). The parameters given here refer to\na low-level method (ndarray(...)
) for instantiating an array.For more information, refer to the
\n\nnumpy
module and examine the\nmethods and attributes of an array.Parameters
\n\n\n
\n\n- (for the __new__ method; see Notes below)
\n- shape (tuple of ints):\nShape of created array.
\n- dtype (data-type, optional):\nAny object that can be interpreted as a numpy data type.
\n- buffer (object exposing buffer interface, optional):\nUsed to fill the array with data.
\n- offset (int, optional):\nOffset of array data in buffer.
\n- strides (tuple of ints, optional):\nStrides of data in memory.
\n- order ({'C', 'F'}, optional):\nRow-major (C-style) or column-major (Fortran-style) order.
\nAttributes
\n\n\n
\n\n- T (ndarray):\nTranspose of the array.
\n- data (buffer):\nThe array's elements, in memory.
\n- dtype (dtype object):\nDescribes the format of the elements in the array.
\n- flags (dict):\nDictionary containing information related to memory use, e.g.,\n'C_CONTIGUOUS', 'OWNDATA', 'WRITEABLE', etc.
\n- flat (numpy.flatiter object):\nFlattened version of the array as an iterator. The iterator\nallows assignments, e.g.,
\nx.flat = 3
(Seendarray.flat
for\nassignment examples; TODO).- imag (ndarray):\nImaginary part of the array.
\n- real (ndarray):\nReal part of the array.
\n- size (int):\nNumber of elements in the array.
\n- itemsize (int):\nThe memory use of each array element in bytes.
\n- nbytes (int):\nThe total number of bytes required to store the array data,\ni.e.,
\nitemsize * size
.- ndim (int):\nThe array's number of dimensions.
\n- shape (tuple of ints):\nShape of the array.
\n- strides (tuple of ints):\nThe step-size required to move from one element to the next in\nmemory. For example, a contiguous
\n(3, 4)
array of type\nint16
in C-order has strides(8, 2)
. This implies that\nto move from element to element in memory requires jumps of 2 bytes.\nTo move from row-to-row, one needs to jump 8 bytes at a time\n(2 * 4
).- ctypes (ctypes object):\nClass containing properties of the array needed for interaction\nwith ctypes.
\n- base (ndarray):\nIf the array is a view into another array, that array is its
\nbase
\n(unless that array is also a view). Thebase
array is where the\narray data is actually stored.See Also
\n\n\n\n
array
: Construct an array.
\nzeros
: Create an array, each element of which is zero.
\nempty
: Create an array, but leave its allocated memory unchanged (i.e.,\nit contains \"garbage\").
\ndtype
: Create a data-type.
\nnumpy.typing.NDArray
: An ndarray alias :term:generic <generic type>
\nw.r.t. itsdtype.type <numpy.dtype.type>
.Notes
\n\nThere are two modes of creating an array using
\n\n__new__
:\n
\n\n- If
\nbuffer
is None, then onlyshape
,dtype
, andorder
\nare used.- If
\nbuffer
is an object exposing the buffer interface, then\nall keywords are interpreted.No
\n\n__init__
method is needed because the array is fully initialized\nafter the__new__
method.Examples
\n\nThese examples illustrate the low-level
\n\nndarray
constructor. Refer\nto theSee Also
section above for easier ways of constructing an\nndarray.First mode,
\n\nbuffer
is None:\n\n\n\n>>> np.ndarray(shape=(2,2), dtype=float, order='F')\narray([[0.0e+000, 0.0e+000], # random\n [ nan, 2.5e-323]])\n
Second mode:
\n\n\n\n", "bases": "numpy.ndarray"}, "pyerrors.input.hadrons.Npr_matrix.__init__": {"fullname": "pyerrors.input.hadrons.Npr_matrix.__init__", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.__init__", "kind": "function", "doc": "\n", "signature": "()"}, "pyerrors.input.hadrons.Npr_matrix.g5H": {"fullname": "pyerrors.input.hadrons.Npr_matrix.g5H", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.g5H", "kind": "variable", "doc": "\n>>> np.ndarray((2,), buffer=np.array([1,2,3]),\n... offset=np.int_().itemsize,\n... dtype=int) # offset = 1*itemsize, i.e. skip first element\narray([2, 3])\n
Gamma_5 hermitean conjugate
\n\nUses the fact that the propagator is gamma5 hermitean, so just the\nin and out momenta of the propagator are exchanged.
\n"}, "pyerrors.input.hadrons.read_ExternalLeg_hd5": {"fullname": "pyerrors.input.hadrons.read_ExternalLeg_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_ExternalLeg_hd5", "kind": "function", "doc": "Read hadrons ExternalLeg hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Bilinear_hd5": {"fullname": "pyerrors.input.hadrons.read_Bilinear_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Bilinear_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons Bilinear hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Fourquark_hd5": {"fullname": "pyerrors.input.hadrons.read_Fourquark_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Fourquark_hd5", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\nRead hadrons FourquarkFullyConnected hdf5 file and output an array of CObs
\n\nParameters
\n\n\n
\n", "signature": "(path, filestem, ens_id, idl=None, vertices=['VA', 'AV']):", "funcdef": "def"}, "pyerrors.input.json": {"fullname": "pyerrors.input.json", "modulename": "pyerrors.input.json", "kind": "module", "doc": "\n"}, "pyerrors.input.json.create_json_string": {"fullname": "pyerrors.input.json.create_json_string", "modulename": "pyerrors.input.json", "qualname": "create_json_string", "kind": "function", "doc": "- path (str):\npath to the files to read
\n- filestem (str):\nnamestem of the files to read
\n- ens_id (str):\nname of the ensemble, required for internal bookkeeping
\n- idl (range):\nIf specified only configurations in the given range are read in.
\n- vertices (list):\nVertex functions to be extracted.
\nGenerate the string for the export of a list of Obs or structures containing Obs\nto a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(ol, description='', indent=1):", "funcdef": "def"}, "pyerrors.input.json.dump_to_json": {"fullname": "pyerrors.input.json.dump_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_to_json", "kind": "function", "doc": "- ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\nExport a list of Obs or structures containing Obs to a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(ol, fname, description='', indent=1, gz=True):", "funcdef": "def"}, "pyerrors.input.json.import_json_string": {"fullname": "pyerrors.input.json.import_json_string", "modulename": "pyerrors.input.json", "qualname": "import_json_string", "kind": "function", "doc": "- ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- fname (str):\nFilename of the output file.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\n- gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
\nReconstruct a list of Obs or structures containing Obs from a json string.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.
\n\nParameters
\n\n\n
\n", "signature": "(json_string, verbose=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.load_json": {"fullname": "pyerrors.input.json.load_json", "modulename": "pyerrors.input.json", "qualname": "load_json", "kind": "function", "doc": "- json_string (str):\njson string containing the data.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\nImport a list of Obs or structures containing Obs from a .json(.gz) file.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.
\n\nParameters
\n\n\n
\n", "signature": "(fname, verbose=True, gz=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.dump_dict_to_json": {"fullname": "pyerrors.input.json.dump_dict_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_dict_to_json", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\nExport a dict of Obs or structures containing Obs to a .json(.gz) file
\n\nParameters
\n\n\n
\n", "signature": "(od, fname, description='', indent=1, reps='DICTOBS', gz=True):", "funcdef": "def"}, "pyerrors.input.json.load_json_dict": {"fullname": "pyerrors.input.json.load_json_dict", "modulename": "pyerrors.input.json", "qualname": "load_json_dict", "kind": "function", "doc": "- od (dict):\nDict of JSON valid structures and objects that will be exported.\nAt the moment, these objects can be either of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
\n- fname (str):\nFilename of the output file.
\n- description (str):\nOptional string that describes the contents of the json file.
\n- indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
\n- reps (str):\nSpecify the structure of the placeholder in exported dict to be reps[0-9]+.
\n- gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
\nImport a dict of Obs or structures containing Obs from a .json(.gz) file.
\n\nThe following structures are supported: Obs, list, numpy.ndarray, Corr
\n\nParameters
\n\n\n
\n", "signature": "(fname, verbose=True, gz=True, full_output=False, reps='DICTOBS'):", "funcdef": "def"}, "pyerrors.input.misc": {"fullname": "pyerrors.input.misc", "modulename": "pyerrors.input.misc", "kind": "module", "doc": "\n"}, "pyerrors.input.misc.read_pbp": {"fullname": "pyerrors.input.misc.read_pbp", "modulename": "pyerrors.input.misc", "qualname": "read_pbp", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- verbose (bool):\nPrint additional information that was written to the file.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\n- full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
\n- reps (str):\nSpecify the structure of the placeholder in imported dict to be reps[0-9]+.
\nRead pbp format from given folder structure. Returns a list of length nrw
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD": {"fullname": "pyerrors.input.openQCD", "modulename": "pyerrors.input.openQCD", "kind": "module", "doc": "\n"}, "pyerrors.input.openQCD.read_rwms": {"fullname": "pyerrors.input.openQCD.read_rwms", "modulename": "pyerrors.input.openQCD", "qualname": "read_rwms", "kind": "function", "doc": "- r_start (list):\nlist which contains the first config to be read for each replicum
\n- r_stop (list):\nlist which contains the last config to be read for each replicum
\nRead rwms format from given folder structure. Returns a list of length nrw
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, version='2.0', names=None, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.extract_t0": {"fullname": "pyerrors.input.openQCD.extract_t0", "modulename": "pyerrors.input.openQCD", "qualname": "extract_t0", "kind": "function", "doc": "- path (str):\npath that contains the data files
\n- prefix (str):\nall files in path that start with prefix are considered as input files.\nMay be used together postfix to consider only special file endings.\nPrefix is ignored, if the keyword 'files' is used.
\n- version (str):\nversion of openQCD, default 2.0
\n- names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
\n- r_start (list):\nlist which contains the first config to be read for each replicum
\n- r_stop (list):\nlist which contains the last config to be read for each replicum
\n- r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
\n- postfix (str):\npostfix of the file to read, e.g. '.ms1' for openQCD-files
\n- files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
\n- print_err (bool):\nPrint additional information that is useful for debugging.
\nExtract t0 from given .ms.dat files. Returns t0 as Obs.
\n\nIt is assumed that all boundary effects have\nsufficiently decayed at x0=xmin.\nThe data around the zero crossing of t^2
\n\n- 0.3\nis fitted with a linear function\nfrom which the exact root is extracted. It is assumed that one measurement is performed for each config.\nIf this is not the case, the resulting idl, as well as the handling\nof r_start, r_stop and r_step is wrong and the user has to correct\nthis in the resulting observable.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop": {"fullname": "pyerrors.input.openQCD.read_qtop", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop", "kind": "function", "doc": "- path (str):\nPath to .ms.dat files
\n- prefix (str):\nEnsemble prefix
\n- dtr_read (int):\nDetermines how many trajectories should be skipped\nwhen reading the ms.dat files.\nCorresponds to dtr_cnfg / dtr_ms in the openQCD input file.
\n- xmin (int):\nFirst timeslice where the boundary\neffects have sufficiently decayed.
\n- spatial_extent (int):\nspatial extent of the lattice, required for normalization.
\n- fit_range (int):\nNumber of data points left and right of the zero\ncrossing to be included in the linear fit. (Default: 5)
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
\n- plaquette (bool):\nIf true extract the plaquette estimate of t0 instead.
\n- names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
\n- files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
\n- plot_fit (bool):\nIf true, the fit for the extraction of t0 is shown together with the data.
\n- assume_thermalization (bool):\nIf True: If the first record divided by the distance between two measurements is larger than\n1, it is assumed that this is due to thermalization and the first measurement belongs\nto the first config (default).\nIf False: The config numbers are assumed to be traj_number // difference
\nRead the topologial charge based on openQCD gradient flow measurements.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, dtr_cnfg=1, version='openQCD', **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_gf_coupling": {"fullname": "pyerrors.input.openQCD.read_gf_coupling", "modulename": "pyerrors.input.openQCD", "qualname": "read_gf_coupling", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files. - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- version (str):\nEither openQCD or sfqcd, depending on the data.
\n- L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
\n- integer_charge (bool):\nIf True, the charge is rounded towards the nearest integer on each config.
\nRead the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.
\n\nNote: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.qtop_projection": {"fullname": "pyerrors.input.openQCD.qtop_projection", "modulename": "pyerrors.input.openQCD", "qualname": "qtop_projection", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files. - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- r_start (list):\nlist which contains the first config to be read for each replicum.
\n- r_stop (list):\nlist which contains the last config to be read for each replicum.
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
\n- postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
\nReturns the projection to the topological charge sector defined by target.
\n\nParameters
\n\n\n
\n", "signature": "(qtop, target=0):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop_sector": {"fullname": "pyerrors.input.openQCD.read_qtop_sector", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop_sector", "kind": "function", "doc": "- path (Obs):\nTopological charge.
\n- target (int):\nSpecifies the topological sector to be reweighted to (default 0)
\nConstructs reweighting factors to a specified topological sector.
\n\nParameters
\n\n\n
\n", "signature": "(path, prefix, c, target=0, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_ms5_xsf": {"fullname": "pyerrors.input.openQCD.read_ms5_xsf", "modulename": "pyerrors.input.openQCD", "qualname": "read_ms5_xsf", "kind": "function", "doc": "- path (str):\npath of the measurement files
\n- prefix (str):\nprefix of the measurement files, e.g.
\n_id0_r0.ms.dat - c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L
\n- target (int):\nSpecifies the topological sector to be reweighted to (default 0)
\n- dtr_cnfg (int):\n(optional) parameter that specifies the number of trajectories\nbetween two configs.\nif it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
\n- steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
\n- version (str):\nversion string of the openQCD (sfqcd) version used to create\nthe ensemble. Default is 2.0. May also be set to sfqcd.
\n- L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
\n- r_start (list):\noffset of the first ensemble, making it easier to match\nlater on with other Obs
\n- r_stop (list):\nlast configurations that need to be read (per replicum)
\n- files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
\n- Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
\nRead data from files in the specified directory with the specified prefix and quark combination extension, and return a
\n\nCorr
object containing the data.Parameters
\n\n\n
\n\n- path (str):\nThe directory to search for the files in.
\n- prefix (str):\nThe prefix to match the files against.
\n- qc (str):\nThe quark combination extension to match the files against.
\n- corr (str):\nThe correlator to extract data for.
\n- sep (str, optional):\nThe separator to use when parsing the replika names.
\n- \n
**kwargs: Additional keyword arguments. The following keyword arguments are recognized:
\n\n\n
- names (List[str]): A list of names to use for the replicas.
\nReturns
\n\n\n
\n\n- Corr: A complex valued
\nCorr
object containing the data read from the files. In case of boudary to bulk correlators.- or
\n- CObs: A complex valued
\nCObs
object containing the data read from the files. In case of boudary to boundary correlators.Raises
\n\n\n
\n", "signature": "(path, prefix, qc, corr, sep='r', **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas": {"fullname": "pyerrors.input.pandas", "modulename": "pyerrors.input.pandas", "kind": "module", "doc": "\n"}, "pyerrors.input.pandas.to_sql": {"fullname": "pyerrors.input.pandas.to_sql", "modulename": "pyerrors.input.pandas", "qualname": "to_sql", "kind": "function", "doc": "- FileNotFoundError: If no files matching the specified prefix and quark combination extension are found in the specified directory.
\n- IOError: If there is an error reading a file.
\n- struct.error: If there is an error unpacking binary data.
\nWrite DataFrame including Obs or Corr valued columns to sqlite database.
\n\nParameters
\n\n\n
\n", "signature": "(df, table_name, db, if_exists='fail', gz=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.read_sql": {"fullname": "pyerrors.input.pandas.read_sql", "modulename": "pyerrors.input.pandas", "qualname": "read_sql", "kind": "function", "doc": "- df (pandas.DataFrame):\nDataframe to be written to the database.
\n- table_name (str):\nName of the table in the database.
\n- db (str):\nPath to the sqlite database.
\n- if exists (str):\nHow to behave if table already exists. Options 'fail', 'replace', 'append'.
\n- gz (bool):\nIf True the json strings are gzipped.
\nExecute SQL query on sqlite database and obtain DataFrame including Obs or Corr valued columns.
\n\nParameters
\n\n\n
\n", "signature": "(sql, db, auto_gamma=False, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.dump_df": {"fullname": "pyerrors.input.pandas.dump_df", "modulename": "pyerrors.input.pandas", "qualname": "dump_df", "kind": "function", "doc": "- sql (str):\nSQL query to be executed.
\n- db (str):\nPath to the sqlite database.
\n- auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
\nExports a pandas DataFrame containing Obs valued columns to a (gzipped) csv file.
\n\nBefore making use of pandas to_csv functionality Obs objects are serialized via the standardized\njson format of pyerrors.
\n\nParameters
\n\n\n
\n", "signature": "(df, fname, gz=True):", "funcdef": "def"}, "pyerrors.input.pandas.load_df": {"fullname": "pyerrors.input.pandas.load_df", "modulename": "pyerrors.input.pandas", "qualname": "load_df", "kind": "function", "doc": "- df (pandas.DataFrame):\nDataframe to be dumped to a file.
\n- fname (str):\nFilename of the output file.
\n- gz (bool):\nIf True, the output is a gzipped csv file. If False, the output is a csv file.
\nImports a pandas DataFrame from a csv.(gz) file in which Obs objects are serialized as json strings.
\n\nParameters
\n\n\n
\n", "signature": "(fname, auto_gamma=False, gz=True):", "funcdef": "def"}, "pyerrors.input.sfcf": {"fullname": "pyerrors.input.sfcf", "modulename": "pyerrors.input.sfcf", "kind": "module", "doc": "\n"}, "pyerrors.input.sfcf.read_sfcf": {"fullname": "pyerrors.input.sfcf.read_sfcf", "modulename": "pyerrors.input.sfcf", "qualname": "read_sfcf", "kind": "function", "doc": "- fname (str):\nFilename of the input file.
\n- auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
\n- gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
\nRead sfcf c format from given folder structure.
\n\nParameters
\n\n\n
\n", "signature": "(\tpath,\tprefix,\tname,\tquarks='.*',\tcorr_type='bi',\tnoffset=0,\twf=0,\twf2=0,\tversion='1.0c',\tcfg_separator='n',\t**kwargs):", "funcdef": "def"}, "pyerrors.input.utils": {"fullname": "pyerrors.input.utils", "modulename": "pyerrors.input.utils", "kind": "module", "doc": "- path (str):\nPath to the sfcf files.
\n- prefix (str):\nPrefix of the sfcf files.
\n- name (str):\nName of the correlation function to read.
\n- quarks (str):\nLabel of the quarks used in the sfcf input file. e.g. \"quark quark\"\nfor version 0.0 this does NOT need to be given with the typical \" - \"\nthat is present in the output file,\nthis is done automatically for this version
\n- corr_type (str):\nType of correlation function to read. Can be\n
\n\n
- 'bi' for boundary-inner
\n- 'bb' for boundary-boundary
\n- 'bib' for boundary-inner-boundary
\n- noffset (int):\nOffset of the source (only relevant when wavefunctions are used)
\n- wf (int):\nID of wave function
\n- wf2 (int):\nID of the second wavefunction\n(only relevant for boundary-to-boundary correlation functions)
\n- im (bool):\nif True, read imaginary instead of real part\nof the correlation function.
\n- names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
\n- ens_name (str):\nreplaces the name of the ensemble
\n- version (str):\nversion of SFCF, with which the measurement was done.\nif the compact output option (-c) was specified,\nappend a \"c\" to the version (e.g. \"1.0c\")\nif the append output option (-a) was specified,\nappend an \"a\" to the version
\n- cfg_separator (str):\nString that separates the ensemble identifier from the configuration number (default 'n').
\n- replica (list):\nlist of replica to be read, default is all
\n- files (list):\nlist of files to be read per replica, default is all.\nfor non-compact output format, hand the folders to be read here.
\n- check_configs:: list of list of supposed configs, eg. [range(1,1000)]\nfor one replicum with 1000 configs
\nUtilities for the input
\n"}, "pyerrors.input.utils.check_idl": {"fullname": "pyerrors.input.utils.check_idl", "modulename": "pyerrors.input.utils", "qualname": "check_idl", "kind": "function", "doc": "Checks if list of configurations is contained in an idl
\n\nParameters
\n\n\n
\n", "signature": "(idl, che):", "funcdef": "def"}, "pyerrors.linalg": {"fullname": "pyerrors.linalg", "modulename": "pyerrors.linalg", "kind": "module", "doc": "\n"}, "pyerrors.linalg.matmul": {"fullname": "pyerrors.linalg.matmul", "modulename": "pyerrors.linalg", "qualname": "matmul", "kind": "function", "doc": "- idl (range or list):\nidl of the current replicum
\n- che (list):\nlist of configurations to be checked against
\nMatrix multiply all operands.
\n\nParameters
\n\n\n
\n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.jack_matmul": {"fullname": "pyerrors.linalg.jack_matmul", "modulename": "pyerrors.linalg", "qualname": "jack_matmul", "kind": "function", "doc": "- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\n- This implementation is faster compared to standard multiplication via the @ operator.
\nMatrix multiply both operands making use of the jackknife approximation.
\n\nParameters
\n\n\n
\n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.einsum": {"fullname": "pyerrors.linalg.einsum", "modulename": "pyerrors.linalg", "qualname": "einsum", "kind": "function", "doc": "- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\n- For large matrices this is considerably faster compared to matmul.
\nWrapper for numpy.einsum
\n\nParameters
\n\n\n
\n", "signature": "(subscripts, *operands):", "funcdef": "def"}, "pyerrors.linalg.inv": {"fullname": "pyerrors.linalg.inv", "modulename": "pyerrors.linalg", "qualname": "inv", "kind": "function", "doc": "- subscripts (str):\nSubscripts for summation (see numpy documentation for details)
\n- operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
\nInverse of Obs or CObs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.cholesky": {"fullname": "pyerrors.linalg.cholesky", "modulename": "pyerrors.linalg", "qualname": "cholesky", "kind": "function", "doc": "Cholesky decomposition of Obs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.det": {"fullname": "pyerrors.linalg.det", "modulename": "pyerrors.linalg", "qualname": "det", "kind": "function", "doc": "Determinant of Obs valued matrices.
\n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.eigh": {"fullname": "pyerrors.linalg.eigh", "modulename": "pyerrors.linalg", "qualname": "eigh", "kind": "function", "doc": "Computes the eigenvalues and eigenvectors of a given hermitian matrix of Obs according to np.linalg.eigh.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.eig": {"fullname": "pyerrors.linalg.eig", "modulename": "pyerrors.linalg", "qualname": "eig", "kind": "function", "doc": "Computes the eigenvalues of a given matrix of Obs according to np.linalg.eig.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.pinv": {"fullname": "pyerrors.linalg.pinv", "modulename": "pyerrors.linalg", "qualname": "pinv", "kind": "function", "doc": "Computes the Moore-Penrose pseudoinverse of a matrix of Obs.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.svd": {"fullname": "pyerrors.linalg.svd", "modulename": "pyerrors.linalg", "qualname": "svd", "kind": "function", "doc": "Computes the singular value decomposition of a matrix of Obs.
\n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.misc": {"fullname": "pyerrors.misc", "modulename": "pyerrors.misc", "kind": "module", "doc": "\n"}, "pyerrors.misc.dump_object": {"fullname": "pyerrors.misc.dump_object", "modulename": "pyerrors.misc", "qualname": "dump_object", "kind": "function", "doc": "Dump object into pickle file.
\n\nParameters
\n\n\n
\n", "signature": "(obj, name, **kwargs):", "funcdef": "def"}, "pyerrors.misc.load_object": {"fullname": "pyerrors.misc.load_object", "modulename": "pyerrors.misc", "qualname": "load_object", "kind": "function", "doc": "- obj (object):\nobject to be saved in the pickle file
\n- name (str):\nname of the file
\n- path (str):\nspecifies a custom path for the file (default '.')
\nLoad object from pickle file.
\n\nParameters
\n\n\n
\n", "signature": "(path):", "funcdef": "def"}, "pyerrors.misc.pseudo_Obs": {"fullname": "pyerrors.misc.pseudo_Obs", "modulename": "pyerrors.misc", "qualname": "pseudo_Obs", "kind": "function", "doc": "- path (str):\npath to the file
\nGenerate an Obs object with given value, dvalue and name for test purposes
\n\nParameters
\n\n\n
\n", "signature": "(value, dvalue, name, samples=1000):", "funcdef": "def"}, "pyerrors.misc.gen_correlated_data": {"fullname": "pyerrors.misc.gen_correlated_data", "modulename": "pyerrors.misc", "qualname": "gen_correlated_data", "kind": "function", "doc": "- value (float):\ncentral value of the Obs to be generated.
\n- dvalue (float):\nerror of the Obs to be generated.
\n- name (str):\nname of the ensemble for which the Obs is to be generated.
\n- samples (int):\nnumber of samples for the Obs (default 1000).
\nGenerate observables with given covariance and autocorrelation times.
\n\nParameters
\n\n\n
\n", "signature": "(means, cov, name, tau=0.5, samples=1000):", "funcdef": "def"}, "pyerrors.mpm": {"fullname": "pyerrors.mpm", "modulename": "pyerrors.mpm", "kind": "module", "doc": "\n"}, "pyerrors.mpm.matrix_pencil_method": {"fullname": "pyerrors.mpm.matrix_pencil_method", "modulename": "pyerrors.mpm", "qualname": "matrix_pencil_method", "kind": "function", "doc": "- means (list):\nlist containing the mean value of each observable.
\n- cov (numpy.ndarray):\ncovariance matrix for the data to be generated.
\n- name (str):\nensemble name for the data to be geneated.
\n- tau (float or list):\ncan either be a real number or a list with an entry for\nevery dataset.
\n- samples (int):\nnumber of samples to be generated for each observable.
\nMatrix pencil method to extract k energy levels from data
\n\nImplementation of the matrix pencil method based on\neq. (2.17) of Y. Hua, T. K. Sarkar, IEEE Trans. Acoust. 38, 814-824 (1990)
\n\nParameters
\n\n\n
\n", "signature": "(corrs, k=1, p=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs": {"fullname": "pyerrors.obs", "modulename": "pyerrors.obs", "kind": "module", "doc": "\n"}, "pyerrors.obs.Obs": {"fullname": "pyerrors.obs.Obs", "modulename": "pyerrors.obs", "qualname": "Obs", "kind": "class", "doc": "- data (list):\ncan be a list of Obs for the analysis of a single correlator, or a list of lists\nof Obs if several correlators are to analyzed at once.
\n- k (int):\nNumber of states to extract (default 1).
\n- p (int):\nmatrix pencil parameter which filters noise. The optimal value is expected between\nlen(data)/3 and 2*len(data)/3. The computation is more expensive the closer p is\nto len(data)/2 but could possibly suppress more noise (default len(data)//2).
\nClass for a general observable.
\n\nInstances of Obs are the basic objects of a pyerrors error analysis.\nThey are initialized with a list which contains arrays of samples for\ndifferent ensembles/replica and another list of same length which contains\nthe names of the ensembles/replica. Mathematical operations can be\nperformed on instances. The result is another instance of Obs. The error of\nan instance can be computed with the gamma_method. Also contains additional\nmethods for output and visualization of the error calculation.
\n\nAttributes
\n\n\n
\n"}, "pyerrors.obs.Obs.__init__": {"fullname": "pyerrors.obs.Obs.__init__", "modulename": "pyerrors.obs", "qualname": "Obs.__init__", "kind": "function", "doc": "- S_global (float):\nStandard value for S (default 2.0)
\n- S_dict (dict):\nDictionary for S values. If an entry for a given ensemble\nexists this overwrites the standard value for that ensemble.
\n- tau_exp_global (float):\nStandard value for tau_exp (default 0.0)
\n- tau_exp_dict (dict):\nDictionary for tau_exp values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
\n- N_sigma_global (float):\nStandard value for N_sigma (default 1.0)
\n- N_sigma_dict (dict):\nDictionary for N_sigma values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
\nInitialize Obs object.
\n\nParameters
\n\n\n
\n", "signature": "(samples, names, idl=None, **kwargs)"}, "pyerrors.obs.Obs.gamma_method": {"fullname": "pyerrors.obs.Obs.gamma_method", "modulename": "pyerrors.obs", "qualname": "Obs.gamma_method", "kind": "function", "doc": "- samples (list):\nlist of numpy arrays containing the Monte Carlo samples
\n- names (list):\nlist of strings labeling the individual samples
\n- idl (list, optional):\nlist of ranges or lists on which the samples are defined
\nEstimate the error and related properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.gm": {"fullname": "pyerrors.obs.Obs.gm", "modulename": "pyerrors.obs", "qualname": "Obs.gm", "kind": "function", "doc": "- S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
\n- tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
\n- N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
\n- fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
\nEstimate the error and related properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.details": {"fullname": "pyerrors.obs.Obs.details", "modulename": "pyerrors.obs", "qualname": "Obs.details", "kind": "function", "doc": "- S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
\n- tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
\n- N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
\n- fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
\nOutput detailed properties of the Obs.
\n\nParameters
\n\n\n
\n", "signature": "(self, ens_content=True):", "funcdef": "def"}, "pyerrors.obs.Obs.reweight": {"fullname": "pyerrors.obs.Obs.reweight", "modulename": "pyerrors.obs", "qualname": "Obs.reweight", "kind": "function", "doc": "- ens_content (bool):\nprint details about the ensembles and replica if true.
\nReweight the obs with given rewighting factors.
\n\nParameters
\n\n\n
\n", "signature": "(self, weight):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero_within_error": {"fullname": "pyerrors.obs.Obs.is_zero_within_error", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero_within_error", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
\nChecks whether the observable is zero within 'sigma' standard errors.
\n\nParameters
\n\n\n
\n", "signature": "(self, sigma=1):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero": {"fullname": "pyerrors.obs.Obs.is_zero", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero", "kind": "function", "doc": "- sigma (int):\nNumber of standard errors used for the check.
\n- Works only properly when the gamma method was run.
\nChecks whether the observable is zero within a given tolerance.
\n\nParameters
\n\n\n
\n", "signature": "(self, atol=1e-10):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_tauint": {"fullname": "pyerrors.obs.Obs.plot_tauint", "modulename": "pyerrors.obs", "qualname": "Obs.plot_tauint", "kind": "function", "doc": "- atol (float):\nAbsolute tolerance (for details see numpy documentation).
\nPlot integrated autocorrelation time for each ensemble.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rho": {"fullname": "pyerrors.obs.Obs.plot_rho", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rho", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nPlot normalized autocorrelation function time for each ensemble.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rep_dist": {"fullname": "pyerrors.obs.Obs.plot_rep_dist", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rep_dist", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nPlot replica distribution for each ensemble with more than one replicum.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_history": {"fullname": "pyerrors.obs.Obs.plot_history", "modulename": "pyerrors.obs", "qualname": "Obs.plot_history", "kind": "function", "doc": "Plot derived Monte Carlo history for each ensemble
\n\nParameters
\n\n\n
\n", "signature": "(self, expand=True):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_piechart": {"fullname": "pyerrors.obs.Obs.plot_piechart", "modulename": "pyerrors.obs", "qualname": "Obs.plot_piechart", "kind": "function", "doc": "- expand (bool):\nshow expanded history for irregular Monte Carlo chains (default: True).
\nPlot piechart which shows the fractional contribution of each\nensemble to the error and returns a dictionary containing the fractions.
\n\nParameters
\n\n\n
\n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.dump": {"fullname": "pyerrors.obs.Obs.dump", "modulename": "pyerrors.obs", "qualname": "Obs.dump", "kind": "function", "doc": "- save (str):\nsaves the figure to a file named 'save' if.
\nDump the Obs to a file 'name' of chosen format.
\n\nParameters
\n\n\n
\n", "signature": "(self, filename, datatype='json.gz', description='', **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.export_jackknife": {"fullname": "pyerrors.obs.Obs.export_jackknife", "modulename": "pyerrors.obs", "qualname": "Obs.export_jackknife", "kind": "function", "doc": "- filename (str):\nname of the file to be saved.
\n- datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
\n- description (str):\nDescription for output file, only relevant for json.gz format.
\n- path (str):\nspecifies a custom path for the file (default '.')
\nExport jackknife samples from the Obs
\n\nReturns
\n\n\n
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sqrt": {"fullname": "pyerrors.obs.Obs.sqrt", "modulename": "pyerrors.obs", "qualname": "Obs.sqrt", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.log": {"fullname": "pyerrors.obs.Obs.log", "modulename": "pyerrors.obs", "qualname": "Obs.log", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.exp": {"fullname": "pyerrors.obs.Obs.exp", "modulename": "pyerrors.obs", "qualname": "Obs.exp", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sin": {"fullname": "pyerrors.obs.Obs.sin", "modulename": "pyerrors.obs", "qualname": "Obs.sin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cos": {"fullname": "pyerrors.obs.Obs.cos", "modulename": "pyerrors.obs", "qualname": "Obs.cos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tan": {"fullname": "pyerrors.obs.Obs.tan", "modulename": "pyerrors.obs", "qualname": "Obs.tan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsin": {"fullname": "pyerrors.obs.Obs.arcsin", "modulename": "pyerrors.obs", "qualname": "Obs.arcsin", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccos": {"fullname": "pyerrors.obs.Obs.arccos", "modulename": "pyerrors.obs", "qualname": "Obs.arccos", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctan": {"fullname": "pyerrors.obs.Obs.arctan", "modulename": "pyerrors.obs", "qualname": "Obs.arctan", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sinh": {"fullname": "pyerrors.obs.Obs.sinh", "modulename": "pyerrors.obs", "qualname": "Obs.sinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cosh": {"fullname": "pyerrors.obs.Obs.cosh", "modulename": "pyerrors.obs", "qualname": "Obs.cosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tanh": {"fullname": "pyerrors.obs.Obs.tanh", "modulename": "pyerrors.obs", "qualname": "Obs.tanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsinh": {"fullname": "pyerrors.obs.Obs.arcsinh", "modulename": "pyerrors.obs", "qualname": "Obs.arcsinh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccosh": {"fullname": "pyerrors.obs.Obs.arccosh", "modulename": "pyerrors.obs", "qualname": "Obs.arccosh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctanh": {"fullname": "pyerrors.obs.Obs.arctanh", "modulename": "pyerrors.obs", "qualname": "Obs.arctanh", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs": {"fullname": "pyerrors.obs.CObs", "modulename": "pyerrors.obs", "qualname": "CObs", "kind": "class", "doc": "- numpy.ndarray: Returns a numpy array of length N + 1 where N is the number of samples\nfor the given ensemble and replicum. The zeroth entry of the array contains\nthe mean value of the Obs, entries 1 to N contain the N jackknife samples\nderived from the Obs. The current implementation only works for observables\ndefined on exactly one ensemble and replicum. The derived jackknife samples\nshould agree with samples from a full jackknife analysis up to O(1/N).
\nClass for a complex valued observable.
\n"}, "pyerrors.obs.CObs.__init__": {"fullname": "pyerrors.obs.CObs.__init__", "modulename": "pyerrors.obs", "qualname": "CObs.__init__", "kind": "function", "doc": "\n", "signature": "(real, imag=0.0)"}, "pyerrors.obs.CObs.gamma_method": {"fullname": "pyerrors.obs.CObs.gamma_method", "modulename": "pyerrors.obs", "qualname": "CObs.gamma_method", "kind": "function", "doc": "Executes the gamma_method for the real and the imaginary part.
\n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.CObs.is_zero": {"fullname": "pyerrors.obs.CObs.is_zero", "modulename": "pyerrors.obs", "qualname": "CObs.is_zero", "kind": "function", "doc": "Checks whether both real and imaginary part are zero within machine precision.
\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs.conjugate": {"fullname": "pyerrors.obs.CObs.conjugate", "modulename": "pyerrors.obs", "qualname": "CObs.conjugate", "kind": "function", "doc": "\n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.derived_observable": {"fullname": "pyerrors.obs.derived_observable", "modulename": "pyerrors.obs", "qualname": "derived_observable", "kind": "function", "doc": "Construct a derived Obs according to func(data, **kwargs) using automatic differentiation.
\n\nParameters
\n\n\n
\n\n- func (object):\narbitrary function of the form func(data, **kwargs). For the\nautomatic differentiation to work, all numpy functions have to have\nthe autograd wrapper (use 'import autograd.numpy as anp').
\n- data (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
\n- num_grad (bool):\nif True, numerical derivatives are used instead of autograd\n(default False). To control the numerical differentiation the\nkwargs of numdifftools.step_generators.MaxStepGenerator\ncan be used.
\n- man_grad (list):\nmanually supply a list or an array which contains the jacobian\nof func. Use cautiously, supplying the wrong derivative will\nnot be intercepted.
\nNotes
\n\nFor simple mathematical operations it can be practical to use anonymous\nfunctions. For the ratio of two observables one can e.g. use
\n\nnew_obs = derived_observable(lambda x: x[0] / x[1], [obs1, obs2])
\n", "signature": "(func, data, array_mode=False, **kwargs):", "funcdef": "def"}, "pyerrors.obs.reweight": {"fullname": "pyerrors.obs.reweight", "modulename": "pyerrors.obs", "qualname": "reweight", "kind": "function", "doc": "Reweight a list of observables.
\n\nParameters
\n\n\n
\n", "signature": "(weight, obs, **kwargs):", "funcdef": "def"}, "pyerrors.obs.correlate": {"fullname": "pyerrors.obs.correlate", "modulename": "pyerrors.obs", "qualname": "correlate", "kind": "function", "doc": "- weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
\n- obs (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
\n- all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
\nCorrelate two observables.
\n\nParameters
\n\n\n
\n\n- obs_a (Obs):\nFirst observable
\n- obs_b (Obs):\nSecond observable
\nNotes
\n\nKeep in mind to only correlate primary observables which have not been reweighted\nyet. The reweighting has to be applied after correlating the observables.\nCurrently only works if ensembles are identical (this is not strictly necessary).
\n", "signature": "(obs_a, obs_b):", "funcdef": "def"}, "pyerrors.obs.covariance": {"fullname": "pyerrors.obs.covariance", "modulename": "pyerrors.obs", "qualname": "covariance", "kind": "function", "doc": "Calculates the error covariance matrix of a set of observables.
\n\nWARNING: This function should be used with care, especially for observables with support on multiple\n ensembles with differing autocorrelations. See the notes below for details.
\n\nThe gamma method has to be applied first to all observables.
\n\nParameters
\n\n\n
\n\n- obs (list or numpy.ndarray):\nList or one dimensional array of Obs
\n- visualize (bool):\nIf True plots the corresponding normalized correlation matrix (default False).
\n- correlation (bool):\nIf True the correlation matrix instead of the error covariance matrix is returned (default False).
\n- smooth (None or int):\nIf smooth is an integer 'E' between 2 and the dimension of the matrix minus 1 the eigenvalue\nsmoothing procedure of hep-lat/9412087 is applied to the correlation matrix which leaves the\nlargest E eigenvalues essentially unchanged and smoothes the smaller eigenvalues to avoid extremely\nsmall ones.
\nNotes
\n\nThe error covariance is defined such that it agrees with the squared standard error for two identical observables\n$$\\operatorname{cov}(a,a)=\\sum_{s=1}^N\\delta_a^s\\delta_a^s/N^2=\\Gamma_{aa}(0)/N=\\operatorname{var}(a)/N=\\sigma_a^2$$\nin the absence of autocorrelation.\nThe error covariance is estimated by calculating the correlation matrix assuming no autocorrelation and then rescaling the correlation matrix by the full errors including the previous gamma method estimate for the autocorrelation of the observables. The covariance at windowsize 0 is guaranteed to be positive semi-definite\n$$\\sum_{i,j}v_i\\Gamma_{ij}(0)v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i,j}v_i\\delta_i^s\\delta_j^s v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i}|v_i\\delta_i^s|^2\\geq 0\\,,$$ for every $v\\in\\mathbb{R}^M$, while such an identity does not hold for larger windows/lags.\nFor observables defined on a single ensemble our approximation is equivalent to assuming that the integrated autocorrelation time of an off-diagonal element is equal to the geometric mean of the integrated autocorrelation times of the corresponding diagonal elements.\n$$\\tau_{\\mathrm{int}, ij}=\\sqrt{\\tau_{\\mathrm{int}, i}\\times \\tau_{\\mathrm{int}, j}}$$\nThis construction ensures that the estimated covariance matrix is positive semi-definite (up to numerical rounding errors).
\n", "signature": "(obs, visualize=False, correlation=False, smooth=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs.import_jackknife": {"fullname": "pyerrors.obs.import_jackknife", "modulename": "pyerrors.obs", "qualname": "import_jackknife", "kind": "function", "doc": "Imports jackknife samples and returns an Obs
\n\nParameters
\n\n\n
\n", "signature": "(jacks, name, idl=None):", "funcdef": "def"}, "pyerrors.obs.merge_obs": {"fullname": "pyerrors.obs.merge_obs", "modulename": "pyerrors.obs", "qualname": "merge_obs", "kind": "function", "doc": "- jacks (numpy.ndarray):\nnumpy array containing the mean value as zeroth entry and\nthe N jackknife samples as first to Nth entry.
\n- name (str):\nname of the ensemble the samples are defined on.
\nCombine all observables in list_of_obs into one new observable
\n\nParameters
\n\n\n
\n\n- list_of_obs (list):\nlist of the Obs object to be combined
\nNotes
\n\nIt is not possible to combine obs which are based on the same replicum
\n", "signature": "(list_of_obs):", "funcdef": "def"}, "pyerrors.obs.cov_Obs": {"fullname": "pyerrors.obs.cov_Obs", "modulename": "pyerrors.obs", "qualname": "cov_Obs", "kind": "function", "doc": "Create an Obs based on mean(s) and a covariance matrix
\n\nParameters
\n\n\n
\n", "signature": "(means, cov, name, grad=None):", "funcdef": "def"}, "pyerrors.roots": {"fullname": "pyerrors.roots", "modulename": "pyerrors.roots", "kind": "module", "doc": "\n"}, "pyerrors.roots.find_root": {"fullname": "pyerrors.roots.find_root", "modulename": "pyerrors.roots", "qualname": "find_root", "kind": "function", "doc": "- mean (list of floats or float):\nN mean value(s) of the new Obs
\n- cov (list or array):\n2d (NxN) Covariance matrix, 1d diagonal entries or 0d covariance
\n- name (str):\nidentifier for the covariance matrix
\n- grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
\nFinds the root of the function func(x, d) where d is an
\n\nObs
.Parameters
\n\n\n
\n\n- d (Obs):\nObs passed to the function.
\n- \n
func (object):\nFunction to be minimized. Any numpy functions have to use the autograd.numpy wrapper.\nExample:
\n\n\n\nimport autograd.numpy as anp\ndef root_func(x, d):\n return anp.exp(-x ** 2) - d\n
- \n
guess (float):\nInitial guess for the minimization.
Returns
\n\n\n
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{"tf": 1.4142135623730951}, "pyerrors.input.openQCD.read_gf_coupling": {"tf": 1.4142135623730951}, "pyerrors.input.openQCD.read_qtop_sector": {"tf": 1.4142135623730951}}, "df": 10}}}}}}}}}}, "pipeline": ["trimmer"], "_isPrebuiltIndex": true}; // mirrored in build-search-index.js (part 1) // Also split on html tags. this is a cheap heuristic, but good enough.- Obs:
\nObs
valued root of the function.