automated photometry pipeline for small to medium-sized observatories
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Updated
Jul 20, 2022 - Python
automated photometry pipeline for small to medium-sized observatories
Gaia science performance simulation toolkit
My astronomy routines
The ASTROnomical POlarimetry and Photometry pipeline
Handling of Science Instrument Aperture Files (SIAF) for space telescopes
FITS to Azimuth/Elevation using Astrometry.net--calibrate and plate scale images
A image classifier that classifies whether a galaxy is spiral, elliptical, or irregular. Built using Tensorflow v2 and Google's inception v3 model.
A fast lost-in-space plate solver for star trackers.
Gathers photometry and astrometry from various ultra-violet, optical, and near-infrared catalogs given a RA, DEC, and Radius by the user. Completed by the user clicking their object overplotted on the catalog images and gathering all of the photometry and astrometry from those various catalogs.
A python module for computing the lateral shift due to atmospheric refraction
Calculates valid ECS coordinates (RA, DEC) from the image coordinates (X, Y) using corrected WCS parameters.
High precision and accuracy astrometric image solving from a guess.
Progress in percentage of the solar system celestial bodies.
This code implements a simplified version of a Gaia-like Global Sphere Reconstruction in Python3.
Extract/Transform/Load (ETL) Framework For Astronomical Catalogs
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