bundles / scipy 1.17.1 / scipy / stats / _stats_py / kurtosis
function
scipy.stats._stats_py:kurtosis
source: /scipy/stats/_stats_py.py :1356
Signature
def kurtosis ( a , axis = 0 , fisher = True , bias = True , nan_policy = propagate , * , keepdims = False ) Summary
Compute the kurtosis (Fisher or Pearson) of a dataset.
Extended Summary
Kurtosis is the fourth central moment divided by the square of the variance. If Fisher's definition is used, then 3.0 is subtracted from the result to give 0.0 for a normal distribution.
If bias is False then the kurtosis is calculated using k statistics to eliminate bias coming from biased moment estimators
Use kurtosistest to see if result is close enough to normal.
Parameters
a: arrayData for which the kurtosis is calculated.
axis: int or None, default: 0If an int, the axis of the input along which to compute the statistic. The statistic of each axis-slice (e.g. row) of the input will appear in a corresponding element of the output. If
None, the input will be raveled before computing the statistic.fisher: bool, optionalIf True, Fisher's definition is used (normal ==> 0.0). If False, Pearson's definition is used (normal ==> 3.0).
bias: bool, optionalIf False, then the calculations are corrected for statistical bias.
nan_policy: {'propagate', 'omit', 'raise'}Defines how to handle input NaNs.
propagate: if a NaN is present in the axis slice (e.g. row) along which the statistic is computed, the corresponding entry of the output will be NaN.omit: NaNs will be omitted when performing the calculation. If insufficient data remains in the axis slice along which the statistic is computed, the corresponding entry of the output will be NaN.raise: if a NaN is present, aValueErrorwill be raised.
keepdims: bool, default: FalseIf this is set to True, the axes which are reduced are left in the result as dimensions with size one. With this option, the result will broadcast correctly against the input array.
Returns
kurtosis: arrayThe kurtosis of values along an axis, returning NaN where all values are equal.
Notes
Beginning in SciPy 1.9, np.matrix inputs (not recommended for new code) are converted to np.ndarray before the calculation is performed. In this case, the output will be a scalar or np.ndarray of appropriate shape rather than a 2D np.matrix. Similarly, while masked elements of masked arrays are ignored, the output will be a scalar or np.ndarray rather than a masked array with mask=False.
Array API Standard Support
kurtosis has experimental support for Python Array API Standard compatible backends in addition to NumPy. Please consider testing these features by setting an environment variable SCIPY_ARRAY_API=1 and providing CuPy, PyTorch, JAX, or Dask arrays as array arguments. The following combinations of backend and device (or other capability) are supported.
==================== ==================== ==================== Library CPU GPU ==================== ==================== ==================== NumPy ✅ n/a CuPy n/a ✅ PyTorch ✅ ✅ JAX ⚠️ no JIT ⚠️ no JIT Dask ⚠️ computes graph n/a ==================== ==================== ====================
See
dev-arrayapifor more information.
Examples
In Fisher's definition, the kurtosis of the normal distribution is zero. In the following example, the kurtosis is close to zero, because it was calculated from the dataset, not from the continuous distribution.import numpy as np from scipy.stats import norm, kurtosis data = norm.rvs(size=1000, random_state=3)✓
kurtosis(data)
✗import matplotlib.pyplot as plt import scipy.stats as stats from scipy.stats import kurtosis✓
x = np.linspace(-5, 5, 100) ax = plt.subplot() distnames = ['laplace', 'norm', 'uniform']✓
for distname in distnames: if distname == 'uniform': dist = getattr(stats, distname)(loc=-2, scale=4) else: dist = getattr(stats, distname) data = dist.rvs(size=1000) kur = kurtosis(data, fisher=True) y = dist.pdf(x) ax.plot(x, y, label="{}, {}".format(distname, round(kur, 3))) ax.legend()✗
Aliases
-
scipy.stats.kurtosis