Galaxy counts and contributions to the background radiation from 1 micron to 1000 microns

Details Galaxy counts and contributions to the background radiation from 1 micron to 1000 microns Galaxy counts and contributions to the background radiation from 1 micron to 1000 microns

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..285f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 2, Aug. 1991, p. 285-310.

Astronomy and Astrophysics

Astronomy

120

Background Radiation, Galactic Evolution, Infrared Radiation, Radio Sources (Astronomy), Spaceborne Telescopes, Angular Resolution, Brightness Distribution, High Resolution

Scientific paper

Predictions are presented for the possible outcome of surveys of the galaxy counts, confusion limits, and contributions to the background radiation in some relevant NIR and mid-IR bands. Predictions were made on the basis of up-to-date models for chemical and photometric evolution of early-type and late-type galaxies, taking into account the luminosity evolution of Seyfert nuclei. It is shown that the models provide a good fit to the recent deep counts in the K band.

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