COBE FIRAS Products

Line Profiles

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Synthetic spectral line profiles are provided for each of the channel and scan modes or merged modes. The synthetic profiles can be used in conjunction with a FIRAS spectrum to calculate line intensities. For a full discussion, see the FIRAS Explanatory Supplement (especially sub-section 8.4 ).


A service of the HEASARC and of the Astrophysics Science Division at NASA/GSFC

HEASARC Director: Dr. Andrew F. Ptak

LAMBDA Director: Dr. Thomas M. Essinger-Hileman

NASA Official: Dr. Thomas M. Essinger-Hileman

Web Curator: Mr. Michael R. Greason