Python CCD photometry
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Updated
Apr 17, 2021 - Fortran
Python CCD photometry
From raw telescope frames to gamma-ray burst physics: image subtraction, PSF photometry, multi-instrument light curves through real filter curves, power-law and afterglowpy jet fits to optical, X-ray and radio data with nested sampling, validated on public ZTF images of GRB 221009A and GRB 210204A.
Extended functionality on the astropy-associated "photutils" photometry package.
A Python module used to reduce monochromatic FITs files and perform basic photometry of stars using PhotUtils (Bradley 2024).
Procesamiento de imagenes astronomicas con astropy
Quality-check and calibrate astrophotography LIGHT frames: star/background stats, satellite-trail detection, HTML report, and an interactive local review server.
PSF-aware isophotal position-angle fitting and GALFIT prep for J-PLUS multi-band galaxy cutouts.
Local MCP server giving AI assistants real astronomical data-reduction tools — FITS inspection, aperture photometry, source detection, light curve fitting, and spectrum extraction, powered by Astropy, Photutils, and Lightkurve.
JWST NIRCam source detection notebook using Astropy and Photutils DAOStarFinder, with image overlays and stellar cutouts.
Quantitative topological comparison between human brain neuronal networks and the cosmic web of galaxies.
Aperture photometry routines for Las Cumbres Observatory images
This repository contains several Python scripts written as a pipeline for raw file sorting (.fits), image reduction (overscanning, trimming, zeroing, etc. w/ flats & biases), & synthetic aperture photometry for spotted stars.
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