Python CCD photometry
-
Updated
Apr 17, 2021 - Fortran
Python CCD photometry
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).
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.
Procesamiento de imagenes astronomicas con astropy
◈ Pipeline astrométrico para detecção de Objetos Próximos da Terra (NEOs) em imagens CCD. Subtração de imagens com ZOGY, calibração WCS utilizando Gaia EDR3, extração de fontes com DAOStarFinder, vinculação de trajetórias e exportação em ADES/XML para submissão ao MPC. Interface web com visualizador FITS (camadas S/R/D/Scorr), galeria de miniaturas
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.
To associate your repository with the photutils topic, visit your repo's landing page and select "manage topics."