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
The Naval Observatory NOVAS C astrometry library, made better
Gaia science performance simulation toolkit
SONIC is an object-oriented optical navigation (OPNAV) toolkit written in MATLAB.
observerly’s lightweight, zero-dependency, fully tree-shakeable, type-safe astrometry library for TypeScript. Sun, Moon, planet and satellite (SGP4) positions, IAU 2006/2000A apparent places, ICRS, ecliptic, galactic and horizontal frame transformations, and transit times, conformance-tested against ERFA (IAU SOFA) to the milliarcsecond.
A fast lost-in-space plate solver for star trackers.
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.
My astronomy routines
Rust astronomical plate solver and image stacking library
Handling of Science Instrument Aperture Files (SIAF) for space telescopes
Modern Fortran implementations of standard models used in fundamental astronomy
The ASTROnomical POlarimetry and Photometry pipeline
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.
Precision astrometry & satellite mechanics in safe, fast Rust.
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
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.
A image classifier that classifies whether a galaxy is spiral, elliptical, or irregular. Built using Tensorflow v2 and Google's inception v3 model.
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