Cited by 15Astronomy and Astrophysical ResearchAstronomical Observations and InstrumentationStellar, planetary, and galactic studies

The FITS Tape Formats: Flexible Image Transport Systems:

Greisen, Eric W., Wells, Donald C., Harten, R. H.·1980·SPIE Proceedings

Abstract

The basic FITS format for the interchange of digital array data was first described in 1979 and is now in use by a wide variety of astronomical institutions. Since the original format was inefficient for use with groups of small arrays, we have now proposed an extension to FITS which supports "arrays" which are irregularly gridded in one or more of the coordinate axes. These formats provide a simple but powerful mechanism for the unambiguous transmission not only of binary image data but also of a virtually unlimited number of auxiliary parameters that may be associated with the data.

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Authors
Greisen, E. W., Wells, D. C., & Harten, R. H.
Affiliations
  • National Radio Astronomy Observatory (US)
  • Kitt Peak National Observatory (US)
  • Netherlands Institute for Radio Astronomy (NL)
Venue
SPIE Proceedings
Publisher
SPIE
Published
1980-11-21
Volume
0264
Pages
298-300
ISSN
0277-786X (ISSN-L)
OpenAlex
W2022680769
Cited by
15
References
0
Citations by year
2026: 1 · 2022: 3 · 2019: 1 · 2015: 7 · 2014: 2
FWCI
0.00
Type
conference paper
Language
en
Open access
closed
Locations
Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE (publishedVersion)
Funders
National Radio Astronomy Observatory
Topics
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
  • Physical Sciences › Engineering › Computational Mechanics › Astronomical Observations and Instrumentation
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
FITS, auxiliary parameter

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