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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

    IRAF V2.15.1a Release Patch Now Available

    (Updated February 21, 2011)

      An IRAF v2.15.1a Patch release is now available from the IRAF anonymous ftp archive at

      This patch is an update of the IRAF v2.15.1 release for all 32- and 64-bit Linux and Mac OSX systems. It is being made available now to address the following specific issue:

      • The earlier v2.15.1 patch introduced a new bug for real FITS images

      In addition, several application-specific bugs that have been discovered since the v2.15.1 release are also fixed, however the minor version increment reflects what we consider to be a minor change to the v2.15.1 release.

      Details of this patch and upgrade instructions may be found in the release announcement.


    IRAF V2.15.1 Release Patch Now Available

    (Updated January 25, 2011)

      An IRAF v2.15.1 Patch release is now available from the IRAF anonymous ftp archive at

      This patch is an update of the IRAF v2.15 release for all 32- and 64-bit Linux and Mac OSX systems. It is being made available now to address the following specific issues:

      • Potential Data Corruption on 64-bit Systems
      • Support for Double-Precision FITS images on 64-bit Systems
      • Remove License Restrictions from the XYACC Compiler
      • Backward-Compatability for NHEDIT tasks

      Details of this patch and upgrade instructions may be found in the release announcement.




    IRAF V2.15 Release Now Available

    (Updated November 21, 2010)


    24-Bit XImtool Now Available

    (Updated September 1, 2009)

    The X11IRAF v2.0 release featuring XImtool support for 24-bit displays is now available as 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 first release and some problems and platform-specific issues might still be found. 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.


    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.