Abstract An important parameter for cosmological studies is the extragalactic far-infrared background radiation. The question we try to answer in this paper is: Which quantitative limits can an analysis of IRAS data put on this background? The answer is not straightforward.
Components of the infrared celestial emission
Advances in Space Research ; 11 , 2 ; 207-212
01.01.1991
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Survey Probe Infrared Celestial Experiment (SPICE)
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