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Welcome to the IRAF Homepage! IRAF is the Image Reduction and Analysis Facility, 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. NOAO is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under cooperative agreement with the National Science Foundation

24-Bit XImtool Available For Testing

The X11IRAF v2.0 release featuring XImtool support for 24-bit displays is now available as a beta release for general use from the following urls:

Limited internal-testing has shown this package is stable enough for wider testing within the user-community, however it should be remembered this is a Beta-release and some problems and platform-specific issues might still be found (but are expected to be easily solved). Known issues (and existing features for those not familiar with XImtool) are outlined in the release notes available at

        ftp://iraf.noao.edu/iraf/x11iraf/Notes-V2.0.html
        ftp://iraf.noao.edu/iraf/x11iraf/Notes-V1.3.html
This release provides only the existing X11IRAF applications with 24-bit X11 display support. See the Notes-V2.0 document above for detailed changes. (Updated November 21, 2008)

IRAF V2.14.1 Patch Now Available



IRAF Support at iraf.net

    Discussions have been underway for a while within NOAO regarding how best to balance the needs of internal projects, the iraf.net support activities, and new projects. The result is a mutual collaboration in which IRAF development is resuming within NOAO on a modest scale, and the community support and development activities at iraf.net will be encouraged and supported for those NOAO employees supporting the site.

    User support remains the primary responsibility of iraf.net. Users are encouraged to Register at that site post questions to the forums. These forums also serve as a searchable online archive of all email sent to the old iraf helpdesk.



Past Features:


What is it? How do I get it?

IRAF is the "Image Reduction and Analysis Facility". The main IRAF distribution includes a good selection of programs for general image processing and graphics, plus a large number of programs for the reduction and analysis of optical and IR astronomy data (the "noao" packages). Other external or layered packages are available for applications such as data acquisition or handling data from other observatories and wavelength regimes such as the Hubble Space Telescope (optical), EUVE (extreme ultra-violet), or ROSAT and AXAF or Chandra (X-ray). These external packages are distributed separately from the main IRAF distribution but can be easily installed. The IRAF system also includes a complete programming environment for scientific applications, which includes a programmable Command Language scripting facility, the IMFORT Fortran/C programming interface, and the full SPP/VOS programming environment in which the portable IRAF system and all applications are written.

IRAF is freely available on all platforms via anonymous ftp to our server at iraf.noao.edu. If you are unsure about whether IRAF can help you, we have a FAQ (frequently-asked questions list) to answer this particular question.


IRAF Project
National Optical Astronomy Observatories
950 North Cherry Avenue
Tucson, Arizona 85719
(520) 318-8000
iraf@noao.edu