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
The Naval Observatory NOVAS C astrometry library, made better
SONIC is an object-oriented optical navigation (OPNAV) toolkit written in MATLAB.
observerly’s lightweight, zero-dependency, type-safe astrometry library for TypeScript. Accurately determine the positions of the Sun, Moon, and planets, handle coordinate transformations with ease, calculate transit times for any celestial object, and integrate precision astronomy into your projects with clean, dependency-free code.
A fast lost-in-space plate solver for star trackers.
My astronomy routines
Cross-platform plate-solving push-to for manual telescopes. ~$50 in hardware, works under heavy urban light pollution. Live tracking to Stellarium, SkySafari, INDI, ASCOM via LX200 or run standalone with built-in catalog. No encoders, no motors, no GOTO mount required.
The ASTROnomical POlarimetry and Photometry pipeline
Modern Fortran implementations of standard models used in fundamental astronomy
FITS File interaction written in Visual Studio C# .Net. JPFITS is not based on any other implementations and is written from the ground-up, consistent with the FITS standard, designed to interact with fits files as object-oriented structures. See the github Wiki link below for more info.
Handling of Science Instrument Aperture Files (SIAF) for space telescopes
Sync astrophotography images from Immich, plate solve them with Astrometry.net, and enrich with searchable celestial metadata.
FITS to Azimuth/Elevation using Astrometry.net--calibrate and plate scale images
Precision astrometry & satellite mechanics in safe, fast Rust.
A image classifier that classifies whether a galaxy is spiral, elliptical, or irregular. Built using Tensorflow v2 and Google's inception v3 model.
observerly's zero-dependency pure Go plate solving library for astronomical images adhering to the WCS and SIP standards
FITS image interaction, world coordinate solving, point source extraction, photometry, etc. See the github Wiki link below for more info. If you require CCDLAB for UVIT, please ensure you have the UVIT Calibration Database which you can find at the CCDLAB Wiki link below.
Wordpress Astrometry.net Plugin
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