A set of functions for analysis of astronomical images
Project description
astromulti
This is a collection of modules for complementing AstroPy in astronomy analysis
fits_actions
: various analysis/modification routines for FITS images
-
remove_axes_34
: removes degenerate 3rd and 4th axes -
bg_filter_I
: filter out background emission using 'un-sharp masking' method developed by Sofue & Reich (1979) -
bg_filter_QU
: modified version of bg_filter_I to work for polarization data as well (-ve values) -
convert_to_JyPerBeam
: convert a FITS file to Jy/beam units (original units in Kelvin) -
regioncut
: get a cutout of a region -
TTdata
: get pixel values of two FITS files with same WCS (for temperature-temperature plots) -
measure_FD
: measure flux density of a region in a fits file -
smooth_fits
: convolve a FITS image to a larger beam size -
smooth_fits_to_commonbeam
: convolve two FITS images to a common beam size -
gauss2Dfit_fits
: perform 2D Gaussian fitting on a point source
linear_fitting
: do least squares fitting to get a line or a plane
new_colormap
: make a new colormap that can be used in plotting data
region_meta
: meta details of a region
simple_funcs
: a collection of simple functions
As the license states, no liability will be accepted. Whatever tests I ran are on Linux, and for my own use case.
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