scipy.stats.recipinvgauss#

scipy.stats.recipinvgauss=<scipy.stats._continuous_distns.recipinvgauss_gen object>[source] #

A reciprocal inverse Gaussian continuous random variable.

As an instance of the rv_continuous class, recipinvgauss 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.

Methods

rvs(mu, loc=0, scale=1, size=1, random_state=None)

Random variates.

pdf(x, mu, loc=0, scale=1)

Probability density function.

logpdf(x, mu, loc=0, scale=1)

Log of the probability density function.

cdf(x, mu, loc=0, scale=1)

Cumulative distribution function.

logcdf(x, mu, loc=0, scale=1)

Log of the cumulative distribution function.

sf(x, mu, loc=0, scale=1)

Survival function (also defined as 1 - cdf, but sf is sometimes more accurate).

logsf(x, mu, loc=0, scale=1)

Log of the survival function.

ppf(q, mu, loc=0, scale=1)

Percent point function (inverse of cdf — percentiles).

isf(q, mu, loc=0, scale=1)

Inverse survival function (inverse of sf).

moment(order, mu, loc=0, scale=1)

Non-central moment of the specified order.

stats(mu, loc=0, scale=1, moments=’mv’)

Mean(‘m’), variance(‘v’), skew(‘s’), and/or kurtosis(‘k’).

entropy(mu, loc=0, scale=1)

(Differential) entropy of the RV.

fit(data)

Parameter estimates for generic data. See scipy.stats.rv_continuous.fit for detailed documentation of the keyword arguments.

expect(func, args=(mu,), 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(mu, loc=0, scale=1)

Median of the distribution.

mean(mu, loc=0, scale=1)

Mean of the distribution.

var(mu, loc=0, scale=1)

Variance of the distribution.

std(mu, loc=0, scale=1)

Standard deviation of the distribution.

interval(confidence, mu, loc=0, scale=1)

Confidence interval with equal areas around the median.

Notes

The probability density function for recipinvgauss is:

\[f(x, \mu) = \frac{1}{\sqrt{2\pi x}} \exp\left(\frac{-(1-\mu x)^2}{2\mu^2x}\right)\]

for \(x \ge 0\).

recipinvgauss takes mu as a shape parameter for \(\mu\).

The probability density above is defined in the "standardized" form. To shift and/or scale the distribution use the loc and scale parameters. Specifically, recipinvgauss.pdf(x, mu, loc, scale) is identically equivalent to recipinvgauss.pdf(y, mu) / scale with y = (x - loc) / scale. Note that shifting the location of a distribution does not make it a "noncentral" distribution; noncentral generalizations of some distributions are available in separate classes.

Examples

>>> importnumpyasnp
>>> fromscipy.statsimport recipinvgauss
>>> importmatplotlib.pyplotasplt
>>> fig, ax = plt.subplots(1, 1)

Get the support:

>>> mu = 0.63
>>> lb, ub = recipinvgauss.support(mu)

Calculate the first four moments:

>>> mean, var, skew, kurt = recipinvgauss.stats(mu, moments='mvsk')

Display the probability density function (pdf):

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

Check accuracy of cdf and ppf:

>>> vals = recipinvgauss.ppf([0.001, 0.5, 0.999], mu)
>>> np.allclose([0.001, 0.5, 0.999], recipinvgauss.cdf(vals, mu))
True

Generate random numbers:

>>> r = recipinvgauss.rvs(mu, size=1000)

And compare the histogram:

>>> ax.hist(r, density=True, bins='auto', histtype='stepfilled', alpha=0.2)
>>> ax.set_xlim([x[0], x[-1]])
>>> ax.legend(loc='best', frameon=False)
>>> plt.show()

../../_images/scipy-stats-recipinvgauss-1.png