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MCMC 2D surface brightness fitting for quasar host galaxies
Python module for calculating pixel-to-pixel RMS noise in astronomical images, taking into account autocorrelation, noise variations in the image weight map, and masking out objects. Intended as a …
Python module and command-line utilities for manipulating small "stamp" images in astronomical FITS files
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Module for manipulating Sextractor source catalogs
5 contributions in the last year
February - September 2018
mmechtley has no activity yet for this period.
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