SigmaClip¶

class
astropy.stats.
SigmaClip
(sigma=3.0, sigma_lower=None, sigma_upper=None, iters=5, cenfunc=<function median>, stdfunc=<function std>)[source] [edit on github]¶ Bases:
object
Class to perform sigma clipping.
The data will be iterated over, each time rejecting points that are discrepant by more than a specified number of standard deviations from a center value. If the data contains invalid values (NaNs or infs), they are automatically masked before performing the sigma clipping.
For a functional interface to sigma clipping, see
sigma_clip()
.Note
scipy.stats.sigmaclip provides a subset of the functionality in this class.
Parameters: sigma : float, optional
The number of standard deviations to use for both the lower and upper clipping limit. These limits are overridden by
sigma_lower
andsigma_upper
, if input. Defaults to 3.sigma_lower : float or
None
, optionalsigma_upper : float or
None
, optionaliters : int or
None
, optionalThe number of iterations to perform sigma clipping, or
None
to clip until convergence is achieved (i.e., continue until the last iteration clips nothing). Defaults to 5.cenfunc : callable, optional
The function used to compute the center for the clipping. Must be a callable that takes in a masked array and outputs the central value. Defaults to the median (
numpy.ma.median
).stdfunc : callable, optional
The function used to compute the standard deviation about the center. Must be a callable that takes in a masked array and outputs a width estimator. Masked (rejected) pixels are those where:
deviation < (sigma_lower * stdfunc(deviation)) deviation > (sigma_upper * stdfunc(deviation))
where:
deviation = data  cenfunc(data [,axis=int])
Defaults to the standard deviation (
numpy.std
).See also
Examples
This example generates random variates from a Gaussian distribution and returns a masked array in which all points that are more than 2 sample standard deviations from the median are masked:
>>> from astropy.stats import SigmaClip >>> from numpy.random import randn >>> randvar = randn(10000) >>> sigclip = SigmaClip(sigma=2, iters=5) >>> filtered_data = sigclip(randvar)
This example sigma clips on a similar distribution, but uses 3 sigma relative to the sample mean, clips until convergence, and does not copy the data:
>>> from astropy.stats import SigmaClip >>> from numpy.random import randn >>> from numpy import mean >>> randvar = randn(10000) >>> sigclip = SigmaClip(sigma=3, iters=None, cenfunc=mean) >>> filtered_data = sigclip(randvar, copy=False)
This example sigma clips along one axis on a similar distribution (with bad points inserted):
>>> from astropy.stats import SigmaClip >>> from numpy.random import normal >>> from numpy import arange, diag, ones >>> data = arange(5) + normal(0., 0.05, (5, 5)) + diag(ones(5)) >>> sigclip = SigmaClip(sigma=2.3) >>> filtered_data = sigclip(data, axis=0)
Note that along the other axis, no points would be masked, as the variance is higher.
Methods Summary
__call__
(data[, axis, copy])Perform sigma clipping on the provided data. Methods Documentation

__call__
(data, axis=None, copy=True)[source] [edit on github]¶ Perform sigma clipping on the provided data.
Parameters: data : arraylike
The data to be sigma clipped.
axis : int or
None
, optionalcopy : bool, optional
Returns: filtered_data :
numpy.ma.MaskedArray
A masked array with the same shape as
data
input, where the points rejected by the algorithm have been masked.
