# scipy.stats.invgauss¶

scipy.stats.invgauss = <scipy.stats.distributions.invgauss_gen object at 0x4203a90>

An inverse Gaussian continuous random variable.

Continuous random variables are defined from a standard form and may require some shape parameters to complete its specification. Any optional keyword parameters can be passed to the methods of the RV object as given below:

Parameters : x : array_like quantiles q : array_like lower or upper tail probability mu : array_like shape parameters loc : array_like, optional location parameter (default=0) scale : array_like, optional scale parameter (default=1) size : int or tuple of ints, optional shape of random variates (default computed from input arguments ) moments : str, optional composed of letters [‘mvsk’] specifying which moments to compute where ‘m’ = mean, ‘v’ = variance, ‘s’ = (Fisher’s) skew and ‘k’ = (Fisher’s) kurtosis. (default=’mv’) Alternatively, the object may be called (as a function) to fix the shape, : location, and scale parameters returning a “frozen” continuous RV object: : rv = invgauss(mu, loc=0, scale=1) : Frozen RV object with the same methods but holding the given shape, location, and scale fixed.

Notes

The probability density function for invgauss is:

```invgauss.pdf(x, mu) = 1 / sqrt(2*pi*x**3) * exp(-(x-mu)**2/(2*x*mu**2))
```

for x > 0.

When mu is too small, evaluating the cumulative density function will be inaccurate due to cdf(mu -> 0) = inf * 0. NaNs are returned for mu <= 0.0028.

Examples

```>>> from scipy.stats import invgauss
>>> numargs = invgauss.numargs
>>> [ mu ] = [0.9,] * numargs
>>> rv = invgauss(mu)
```

Display frozen pdf

```>>> x = np.linspace(0, np.minimum(rv.dist.b, 3))
>>> h = plt.plot(x, rv.pdf(x))
```

Check accuracy of cdf and ppf

```>>> prb = invgauss.cdf(x, mu)
>>> h = plt.semilogy(np.abs(x - invgauss.ppf(prb, mu)) + 1e-20)
```

Random number generation

```>>> R = invgauss.rvs(mu, size=100)
```

Methods

 rvs(mu, loc=0, scale=1, size=1) 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 density function. logcdf(x, mu, loc=0, scale=1) Log of the cumulative density function. sf(x, mu, loc=0, scale=1) Survival function (1-cdf — 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(n, mu, loc=0, scale=1) Non-central moment of order n 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, mu, loc=0, scale=1) Parameter estimates for generic data. expect(func, 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(alpha, mu, loc=0, scale=1) Endpoints of the range that contains alpha percent of the distribution

#### Previous topic

scipy.stats.invgamma

#### Next topic

scipy.stats.invweibull