scipy.special.chdtr#
- scipy.special.chdtr(v, x, out=None) = <ufunc 'chdtr'>#
Chi square cumulative distribution function.
Returns the area under the left tail (from 0 to x) of the Chi square probability density function with v degrees of freedom:
\[\frac{1}{2^{v/2} \Gamma(v/2)} \int_0^x t^{v/2 - 1} e^{-t/2} dt\]Here \(\Gamma\) is the Gamma function; see
gamma. This integral can be expressed in terms of the regularized lower incomplete gamma functiongammaincasgammainc(v / 2, x / 2). [1]- Parameters:
- varray_like
Degrees of freedom.
- xarray_like
Upper bound of the integral.
- outndarray, optional
Optional output array for the function results.
- Returns:
- scalar or ndarray
Values of the cumulative distribution function.
Notes
Array API Standard Support
chdtrhas support for Python Array API Standard compatible backends in addition to NumPy. The following combinations of backend and device (or other capability) are supported.Library
CPU
GPU
NumPy
✅
n/a
CuPy
n/a
✅
PyTorch
✅
✅
JAX
✅
✅
Dask
✅
n/a
For the NumPy backend, this function supports all NumPy ufunc keyword arguments. Other backends may support
out, but none of the other ufunc kwargs.outis typically supported for CuPy and PyTorch, but not currently in cases where SciPy relies on a generic Array API implementation or, for PyTorch on CPU, falls back to the NumPy backend.outis never supported for JAX because JAX arrays are immutable.chdtrdoes not currently supportoutfor the PyTorch backend.See Support for the array API standard for more information.
References
[1]Chi-Square distribution, https://www.itl.nist.gov/div898/handbook/eda/section3/eda3666.htm
Examples
>>> import numpy as np >>> import scipy.special as sc
It can be expressed in terms of the regularized lower incomplete gamma function.
>>> v = 1 >>> x = np.arange(4) >>> sc.chdtr(v, x) array([0. , 0.68268949, 0.84270079, 0.91673548]) >>> sc.gammainc(v / 2, x / 2) array([0. , 0.68268949, 0.84270079, 0.91673548])