Cited by 206Astronomy and Astrophysical ResearchAstronomical Observations and InstrumentationStellar, planetary, and galactic studies

Representations of world coordinates in FITS

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Greisen, E. W., Calabretta, M. R.·2002·Astronomy & Astrophysics

Abstract

The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image coordinates. Building on conventions in wide use within astronomy, this paper proposes general extensions to the original methods for describing the world coordinates of FITS data. In subsequent papers, we apply these general conventions to the methods by which spherical coordinates may be projected onto a two-dimensional plane and to frequency/wavelength/velocity coordinates.

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Crossref · 10.1051/0004-6361:20021326

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  • Header sections store essential metadata as keyword/value pairs, including observational parameters, processing history, WCS information, and flux calibration.

    “Critically, the header sections store essential metadata as keyword / value pairs. This includes observational parameters (telescope telemetry, instrument configuration, exposure time, filters), processing history (calibration steps, software versions), and arguably most importantly, the World Coordinate System (WCS) information (Greisen and Calabretta, 2002; Calabretta and Greisen, 2002) and flux”

    From A high-throughput AES-GCM implementation on GPUs for secure, policy-based access to massive astronomical catalogs (2026) · cites this paper as Greisen and Calabretta, 2002

    The Introduction describes FITS headers as keyword-equals-value records and says this paper defines WCS keywords. Section 5.4 gives an exposure-time keyword as an example. The cited paper does not establish the full list of header contents attributed to it, particularly processing history, software versions, and flux calibration. Page numbers are unavailable in our copy. (LLM, conf=0.88)

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Research works printed but not linked: 2

  1. Adobe Systems, Inc. 1999, PostScript Language Reference Manual, Third ed. (Addison-Wesley Publishing Company, Inc.), Reading, Massachusetts (see especially pages 293-296)
  2. McNally, D. (ed.) 1988, Transactions of the IAU, Proceedings of the Twentieth General Assembly (Dordrecht: Kluwer)

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Authors
Greisen, E. W., & Calabretta, M. R.
Affiliations
  • National Radio Astronomy Observatory (US)
  • Australia Telescope National Facility (AU)
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2002-11-18
Volume
395
Issue
3
Pages
1061-1075
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2051633863
Cited by
206
References
1
Citations by year
2026: 11 · 2025: 8 · 2024: 12 · 2023: 12 · 2022: 16 · 2021: 7 · 2020: 12 · 2019: 6 · 2018: 8 · 2017: 12 · 2016: 18 · 2015: 13 · 2014: 11 · 2013: 6 · 2012: 8
FWCI
7.34
Type
journal article
Language
en
Open access
Locations
  • Astronomy and Astrophysics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Aeronautics and Space Administration
  • Space Telescope Science Institute
  • Goddard Space Flight Center
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 format, world coordinates, coordinate systems, spherical projection

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