I want to fit a gamma distribution to my data, which I do using this
import scipy.stats as ss
import scipy as sp
import numpy as np
import os
import matplotlib.pyplot as plt
alpha = []
beta = []
loc = []
data = np.loadtxt(data)
fit_alpha, fit_loc, fit_beta = ss.gamma.fit(data, floc=0, fscale=1)
I want to keep one of the parameters to the gamma distribution as a variable (say the shape), and fix one of the parameters (say scale=1
). However, if I keep the loc variable as zero, I am not able to fix the scale at one. Is there some workaround for this? Can I not parametrize the gamma distribution using only the shape and scale?
To fit the gamma distribution to data and find parameter estimates, use gamfit , fitdist , or mle . Unlike gamfit and mle , which return parameter estimates, fitdist returns the fitted probability distribution object GammaDistribution . The object properties a and b store the parameter estimates.
A gamma continuous random variable. As an instance of the rv_continuous class, gamma object inherits from it a collection of generic methods (see below for the full list), and completes them with details specific for this particular distribution. See also erlang , expon. Notes.
In a comment I said you have run into a bug in the gamma
distribution--it does not let you fix both the location and the scale. The bug was fixed in scipy 0.13, but if you can't upgrade, you can work around the bug by using the fit
method of the class rv_continuous
, which is the parent class of gamma
:
In [22]: from scipy.stats import rv_continuous, gamma
In [23]: x = gamma.rvs(2.5, loc=0, scale=4, size=1000) # A test sample.
In [24]: rv_continuous.fit(gamma, x, floc=0, fscale=4)
Out[24]: (2.5335837650122608, 0, 4)
Looking at the implementation of gamma.fit:
def fit(self, data, *args, **kwds):
floc = kwds.get('floc', None)
if floc == 0:
xbar = ravel(data).mean()
logx_bar = ravel(log(data)).mean()
s = log(xbar) - logx_bar
def func(a):
return log(a) - special.digamma(a) - s
aest = (3-s + math.sqrt((s-3)**2 + 24*s)) / (12*s)
xa = aest*(1-0.4)
xb = aest*(1+0.4)
a = optimize.brentq(func, xa, xb, disp=0)
scale = xbar / a
return a, floc, scale
else:
return super(gamma_gen, self).fit(data, *args, **kwds)
If you put floc=None, it will call the fit function of the parent class (which is rv_continuous) and you can fix the scale.
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