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These images were produced by dividing the 0.5° x 0.5° beam data
contained in the standard Zodiacal Observation
History File into the three separate sky coverages
(HCONs) and assembling them into three maps with
an Aitoff equal area projection
in Galactic coordinates. Two fields of each sky coverage were
produced, one centered on the Galactic center and one on the Galactic
anticenter, yielding a total of six images per wavelength band. The
files are in FITS format. For more information see the Explanatory Supplement.
Reference:
Infrared Astronomical Satellite (IRAS) Catalogs and Atlases, vol. 1,
Explanatory Supplement, 1988, ed. C. Beichman, et al., NASA RP-1190
(Washington, DC: GPO)
Version and release date: 1.0, 1984 Nov 26
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