scipy.stats.t¶
-
scipy.stats.
t
= <scipy.stats._continuous_distns.t_gen object>[source]¶ A Student’s t continuous random variable.
For the noncentral t distribution, see
nct
.As an instance of the
rv_continuous
class,t
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
Notes
The probability density function for
t
is:\[f(x, \nu) = \frac{\Gamma((\nu+1)/2)} {\sqrt{\pi \nu} \Gamma(\nu/2)} (1+x^2/\nu)^{-(\nu+1)/2}\]where \(x\) is a real number and the degrees of freedom parameter \(\nu\) (denoted
df
in the implementation) satisfies \(\nu > 0\). \(\Gamma\) is the gamma function (scipy.special.gamma
).The probability density above is defined in the “standardized” form. To shift and/or scale the distribution use the
loc
andscale
parameters. Specifically,t.pdf(x, df, loc, scale)
is identically equivalent tot.pdf(y, df) / scale
withy = (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
>>> from scipy.stats import t >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(1, 1)
Calculate the first four moments:
>>> df = 2.74 >>> mean, var, skew, kurt = t.stats(df, moments='mvsk')
Display the probability density function (
pdf
):>>> x = np.linspace(t.ppf(0.01, df), ... t.ppf(0.99, df), 100) >>> ax.plot(x, t.pdf(x, df), ... 'r-', lw=5, alpha=0.6, label='t 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 = t(df) >>> ax.plot(x, rv.pdf(x), 'k-', lw=2, label='frozen pdf')
Check accuracy of
cdf
andppf
:>>> vals = t.ppf([0.001, 0.5, 0.999], df) >>> np.allclose([0.001, 0.5, 0.999], t.cdf(vals, df)) True
Generate random numbers:
>>> r = t.rvs(df, 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, loc=0, scale=1, size=1, random_state=None)
Random variates.
pdf(x, df, loc=0, scale=1)
Probability density function.
logpdf(x, df, loc=0, scale=1)
Log of the probability density function.
cdf(x, df, loc=0, scale=1)
Cumulative distribution function.
logcdf(x, df, loc=0, scale=1)
Log of the cumulative distribution function.
sf(x, df, loc=0, scale=1)
Survival function (also defined as
1 - cdf
, but sf is sometimes more accurate).logsf(x, df, loc=0, scale=1)
Log of the survival function.
ppf(q, df, loc=0, scale=1)
Percent point function (inverse of
cdf
— percentiles).isf(q, df, loc=0, scale=1)
Inverse survival function (inverse of
sf
).moment(n, df, loc=0, scale=1)
Non-central moment of order n
stats(df, loc=0, scale=1, moments=’mv’)
Mean(‘m’), variance(‘v’), skew(‘s’), and/or kurtosis(‘k’).
entropy(df, 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=(df,), 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, loc=0, scale=1)
Median of the distribution.
mean(df, loc=0, scale=1)
Mean of the distribution.
var(df, loc=0, scale=1)
Variance of the distribution.
std(df, loc=0, scale=1)
Standard deviation of the distribution.
interval(alpha, df, loc=0, scale=1)
Endpoints of the range that contains fraction alpha [0, 1] of the distribution