86 KiB
Basic pyerrors example¶
Import numpy, matplotlib and pyerrors.
import numpy as np
import matplotlib
import matplotlib.pyplot as plt
import pyerrors as pe
plt.style.use('./base_style.mplstyle')
usetex = matplotlib.checkdep_usetex(True)
plt.rc('text', usetex=usetex)
We use numpy to generate some fake data
test_sample1 = np.random.normal(2.0, 0.5, 1000)
test_sample2 = np.random.normal(1.0, 0.1, 1000)
From this we can construct Obs, which are the basic object of pyerrors. For each sample we give to the obs, we also have to specify an ensemble/replica name. In this example we assume that both datasets originate from the same gauge field ensemble labeled 'ens1'.
obs1 = pe.Obs([test_sample1], ['ensemble1'])
obs2 = pe.Obs([test_sample2], ['ensemble1'])
We can now combine these two observables into a third one:
obs3 = np.log(obs1 ** 2 / obs2 ** 4)
pyerrors overloads all basic math operations, the user can work with these Obs as if they were real numbers. The proper error propagation is performed in the background via automatic differentiation.
If we are now interested in the error of obs3, we can use the gamma_method to compute it and then print the object to the notebook
obs3.gamma_method()
print(obs3)
With the method details we can take a look at the integrated autocorrelation time estimated by the automatic windowing procedure as well as the detailed content of the Obs object.
obs3.details()
As expected the random data from numpy exhibits no autocorrelation ($\tau_\text{int}\,\approx0.5$). It can still be interesting to have a look at the window size dependence of the integrated autocorrelation time
obs3.plot_tauint()
This figure shows the windowsize dependence of the integrated autocorrelation time. The vertical line signalizes the window chosen by the automatic windowing procedure with $S=2.0$. Choosing a larger windowsize would not significantly alter $\tau_\text{int}$, so everything seems to be correct here.
Correlated data¶
We can now generate fake data with a given covariance matrix and integrated autocorrelation times:
cov = np.array([[0.5, -0.2], [-0.2, 0.3]]) # Covariance matrix
tau = [4, 8] # Autocorrelation times
c_obs1, c_obs2 = pe.misc.gen_correlated_data([2.8, 2.1], cov, 'ens1', tau)
and once again combine the two Obs to a new one with arbitrary math operations
c_obs3 = np.sin(c_obs1 / c_obs2 - 1)
c_obs3.gamma_method()
c_obs3.details()
This time we see a significant autocorrelation so it is worth to have a closer look at the normalized autocorrelation function (rho) and the integrated autocorrelation time
c_obs3.plot_rho()
c_obs3.plot_tauint()
We can now redo the error analysis and alter the value of S or attach a tail to the autocorrelation function via the parameter tau_exp to take into account long range autocorrelations
c_obs3.gamma_method(tau_exp=20)
c_obs3.details()
c_obs3.plot_tauint()