LSST Science Pipelines

Forum
Docs
LSST.org →

Navigation

next »
« previous |
LSST Science Pipelines »
lsst.analysis.tools »
nanSigmaMad

nanSigmaMad¶

lsst.analysis.tools.nanSigmaMad(vector: ndarray[Any, dtype[_ScalarType_co]]) → Scalar¶: Return the sigma_MAD of a vector.

On this page

nanSigmaMad
- nanSigmaMad()

Last built Dec 19, 2024.

Created using Sphinx 6.2.1. Page design is based on Astropy's bootstrap-astropy theme in astropy-helpers.
LSST documentation is proudly served through the Fastly CDN.

© Copyright 2015-2024 LSST contributors.

Financial support for LSST comes from the National Science Foundation (NSF) through Cooperative Agreement No. 1258333, the Department of Energy (DOE) Office of Science under Contract No. DE-AC02-76SF00515, and private funding raised by the LSST Corporation. The NSF-funded LSST Project Office for construction was established as an operating center under management of the Association of Universities for Research in Astronomy (AURA). The DOE-funded effort to build the LSST camera is managed by the SLAC National Accelerator Laboratory (SLAC).