scipy.stats.gausshyper = <scipy.stats._continuous_distns.gausshyper_gen object>[source]

A Gauss hypergeometric continuous random variable.

As an instance of the rv_continuous class, gausshyper 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.


The probability density function for gausshyper is:

\[f(x, a, b, c, z) = C x^{a-1} (1-x)^{b-1} (1+zx)^{-c}\]

for \(0 \le x \le 1\), \(a > 0\), \(b > 0\), and \(C = \frac{1}{B(a, b) F[2, 1](c, a; a+b; -z)}\)

gausshyper takes \(a\), \(b\), \(c\) and \(z\) as shape parameters.

The probability density above is defined in the “standardized” form. To shift and/or scale the distribution use the loc and scale parameters. Specifically, gausshyper.pdf(x, a, b, c, z, loc, scale) is identically equivalent to gausshyper.pdf(y, a, b, c, z) / scale with y = (x - loc) / scale.


>>> from scipy.stats import gausshyper
>>> import matplotlib.pyplot as plt
>>> fig, ax = plt.subplots(1, 1)

Calculate a few first moments:

>>> a, b, c, z = 13.8, 3.12, 2.51, 5.18
>>> mean, var, skew, kurt = gausshyper.stats(a, b, c, z, moments='mvsk')

Display the probability density function (pdf):

>>> x = np.linspace(gausshyper.ppf(0.01, a, b, c, z),
...                 gausshyper.ppf(0.99, a, b, c, z), 100)
>>> ax.plot(x, gausshyper.pdf(x, a, b, c, z),
...        'r-', lw=5, alpha=0.6, label='gausshyper pdf')

Alternatively, the distribution object can be called (as a function) to fix the shape, location and scale parameters. This returns a “frozen” RV object holding the given parameters fixed.

Freeze the distribution and display the frozen pdf:

>>> rv = gausshyper(a, b, c, z)
>>> ax.plot(x, rv.pdf(x), 'k-', lw=2, label='frozen pdf')

Check accuracy of cdf and ppf:

>>> vals = gausshyper.ppf([0.001, 0.5, 0.999], a, b, c, z)
>>> np.allclose([0.001, 0.5, 0.999], gausshyper.cdf(vals, a, b, c, z))

Generate random numbers:

>>> r = gausshyper.rvs(a, b, c, z, size=1000)

And compare the histogram:

>>> ax.hist(r, density=True, histtype='stepfilled', alpha=0.2)
>>> ax.legend(loc='best', frameon=False)


rvs(a, b, c, z, loc=0, scale=1, size=1, random_state=None) Random variates.
pdf(x, a, b, c, z, loc=0, scale=1) Probability density function.
logpdf(x, a, b, c, z, loc=0, scale=1) Log of the probability density function.
cdf(x, a, b, c, z, loc=0, scale=1) Cumulative distribution function.
logcdf(x, a, b, c, z, loc=0, scale=1) Log of the cumulative distribution function.
sf(x, a, b, c, z, loc=0, scale=1) Survival function (also defined as 1 - cdf, but sf is sometimes more accurate).
logsf(x, a, b, c, z, loc=0, scale=1) Log of the survival function.
ppf(q, a, b, c, z, loc=0, scale=1) Percent point function (inverse of cdf — percentiles).
isf(q, a, b, c, z, loc=0, scale=1) Inverse survival function (inverse of sf).
moment(n, a, b, c, z, loc=0, scale=1) Non-central moment of order n
stats(a, b, c, z, loc=0, scale=1, moments=’mv’) Mean(‘m’), variance(‘v’), skew(‘s’), and/or kurtosis(‘k’).
entropy(a, b, c, z, loc=0, scale=1) (Differential) entropy of the RV.
fit(data, a, b, c, z, loc=0, scale=1) Parameter estimates for generic data.
expect(func, args=(a, b, c, z), loc=0, scale=1, lb=None, ub=None, conditional=False, **kwds) Expected value of a function (of one argument) with respect to the distribution.
median(a, b, c, z, loc=0, scale=1) Median of the distribution.
mean(a, b, c, z, loc=0, scale=1) Mean of the distribution.
var(a, b, c, z, loc=0, scale=1) Variance of the distribution.
std(a, b, c, z, loc=0, scale=1) Standard deviation of the distribution.
interval(alpha, a, b, c, z, loc=0, scale=1) Endpoints of the range that contains alpha percent of the distribution

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