scipy.stats.ncx2

scipy.stats.ncx2 = <scipy.stats._continuous_distns.ncx2_gen object>

A non-central chi-squared continuous random variable.

As an instance of the rv_continuous class, ncx2 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.

Notes

The probability density function for ncx2 is:

\[f(x, k, \lambda) = \frac{1}{2} \exp(-(\lambda+x)/2) (x/\lambda)^{(k-2)/4} I_{(k-2)/2}(\sqrt{\lambda x})\]

for \(x > 0\) and \(k, \lambda > 0\). \(k\) specifies the degrees of freedom (denoted df in the implementation) and \(\lambda\) is the non-centrality parameter (denoted nc in the implementation). \(I_\nu\) denotes the modified Bessel function of first order of degree \(\nu\) (scipy.special.iv).

ncx2 takes df and nc 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, ncx2.pdf(x, df, nc, loc, scale) is identically equivalent to ncx2.pdf(y, df, nc) / scale with y = (x - loc) / scale.

Examples

>>> from scipy.stats import ncx2
>>> import matplotlib.pyplot as plt
>>> fig, ax = plt.subplots(1, 1)

Calculate a few first moments:

>>> df, nc = 21, 1.06
>>> mean, var, skew, kurt = ncx2.stats(df, nc, moments='mvsk')

Display the probability density function (pdf):

>>> x = np.linspace(ncx2.ppf(0.01, df, nc),
...                 ncx2.ppf(0.99, df, nc), 100)
>>> ax.plot(x, ncx2.pdf(x, df, nc),
...        'r-', lw=5, alpha=0.6, label='ncx2 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 = ncx2(df, nc)
>>> ax.plot(x, rv.pdf(x), 'k-', lw=2, label='frozen pdf')

Check accuracy of cdf and ppf:

>>> vals = ncx2.ppf([0.001, 0.5, 0.999], df, nc)
>>> np.allclose([0.001, 0.5, 0.999], ncx2.cdf(vals, df, nc))
True

Generate random numbers:

>>> r = ncx2.rvs(df, nc, size=1000)

And compare the histogram:

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

Methods

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