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FITS Image Format

AIPS - Astronomical Image Processing System
[open source - Unix, and VMS] A software package for interactive (and, optionally, batch) calibration and editing of radio interferometric data and for the calibration, construction, display and analysis of astronomical images made from those data using Fourier synthesis methods. (infos)

IRAF - Image Reduction and Analysis Facility
[open source - Unix, OpenVMS] A general-purpose software system for the reduction and analysis of astronomical data. IRAF is written and supported by the IRAF programming group at the National Optical Astronomy Observatories (NOAO) in Tucson, Arizona. (infos)

ESO-MIDAS: Image Data Analysis System
[open source - Linux/Unix, VAX/VMS/OpenVMS] General tools for image processing and data reduction with emphasis on astronomical applications including stellar and surface photometry, image sharpening and decomposition, as well as imaging and special reduction packages for ESO instrumentation. (infos)

AIPS++
[open source - Unix, WinNT] The next generation AIPS software. (infos)

GIPSY - Groningen Image Processing System
[open source - Unix] A highly interactive software system for the reduction and display of astronomical data. (infos)

SuperFix/MegaFix
[commercial - DOS, Win3.1] CCD image processing software for amateur astronomers. Handles most file and camera formats. Allows tricolor imaging and 'track-and-stack as well'. (infos)

IDL - Interactive Data Language
[commercial - multiplatform] Data analysis, visualization, and cross-platform application development software. (infos)

PV-WAVE
[commercial - multiplatform] Advanced visual data analysis software. (infos)

MaxIm DL
[commercial, demo available - Win95/98/NT/2000] Image processing and CCD camera control software for astronomical imaging. Supports Apogee, Celestron, FLI, HiSIS, Meade, SBIG, and Starlight Xpress CCD cameras; video cameras, autoguiders, and filter wheels. ASCOM compliant. (infos)

Seeing Simulation and Deconvolution
GPL implementation of a seeing simulator and deconvolution via Cross-spectrum and Bi-spectrum. Features operational information, sample output and download. (infos)

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