11.6.9. astroML.stats.trunc_exp

astroML.stats.trunc_exp(*args, **kwds)

A truncated positive exponential continuous random variable.

The probability distribution is:

p(x) ~ exp(k * x)   between a and b
     = 0            otherwise

The arguments are (a, b, k)

As an instance of the rv_continuous class, trunc_exp 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.

Examples

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

Calculate a few first moments:

>>> a, b, k = 
>>> mean, var, skew, kurt = trunc_exp.stats(a, b, k, moments='mvsk')

Display the probability density function (pdf):

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

Check accuracy of cdf and ppf:

>>> vals = trunc_exp.ppf([0.001, 0.5, 0.999], a, b, k)
>>> np.allclose([0.001, 0.5, 0.999], trunc_exp.cdf(vals, a, b, k))
True

Generate random numbers:

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

11.6.8. astroML.stats.bivariate_normal 11.6.10. astroML.stats.linear