scipy.stats.burr12 = <scipy.stats._continuous_distns.burr12_gen object at 0x2b909bab9f90>[source]

A Burr (Type XII) continuous random variable.

As an instance of the rv_continuous class, burr12 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

a special case of either burr or burr12 with d = 1
Burr Type III distribution


The probability density function for burr is:

burr12.pdf(x, c, d) = c * d * x**(c-1) * (1+x**(c))**(-d-1)

for x > 0.

burr12 takes c and d as shape parameters.

This is the PDF corresponding to the twelfth CDF given in Burr’s list; specifically, it is equation (20) in Burr’s paper [R500].

The probability density above is defined in the “standardized” form. To shift and/or scale the distribution use the loc and scale parameters. Specifically, burr12.pdf(x, c, d, loc, scale) is identically equivalent to burr12.pdf(y, c, d) / scale with y = (x - loc) / scale.

The Burr type 12 distribution is also sometimes referred to as the Singh-Maddala distribution from NIST [R501].


[R500](1, 2) Burr, I. W. “Cumulative frequency functions”, Annals of Mathematical Statistics, 13(2), pp 215-232 (1942).
[R501](1, 2)


>>> from scipy.stats import burr12
>>> import matplotlib.pyplot as plt
>>> fig, ax = plt.subplots(1, 1)

Calculate a few first moments:

>>> c, d = 10, 4
>>> mean, var, skew, kurt = burr12.stats(c, d, moments='mvsk')

Display the probability density function (pdf):

>>> x = np.linspace(burr12.ppf(0.01, c, d),
...                 burr12.ppf(0.99, c, d), 100)
>>> ax.plot(x, burr12.pdf(x, c, d),
...        'r-', lw=5, alpha=0.6, label='burr12 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 = burr12(c, d)
>>> ax.plot(x, rv.pdf(x), 'k-', lw=2, label='frozen pdf')

Check accuracy of cdf and ppf:

>>> vals = burr12.ppf([0.001, 0.5, 0.999], c, d)
>>> np.allclose([0.001, 0.5, 0.999], burr12.cdf(vals, c, d))

Generate random numbers:

>>> r = burr12.rvs(c, d, size=1000)

And compare the histogram:

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

(Source code)



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

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