Deep galaxy count predictions in the radio, infrared, and X-ray spectral bands

Details Deep galaxy count predictions in the radio, infrared, and X-ray spectral bands Deep galaxy count predictions in the radio, infrared, and X-ray spectral bands

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...408l...1t&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 408, no. 1, p. L1-L4.

Astronomy and Astrophysics

Astronomy

15

Astronomical Spectroscopy, Diffuse Radiation, Galactic Evolution, Sky Surveys (Astronomy), Starburst Galaxies, Infrared Astronomy, Radio Astronomy, X Ray Astronomy

Scientific paper

The existence of a dominant population of strongly evolving starburst sources at moderate redshift is a plausible explanation for the excess number of faint blue galaxies detected in deep sky surveys. Multiwavelength observations at faint magnitudes would allow the existence of such a population to be confirmed. We use observed luminosity correlations and physical properties of known starburst galaxies to predict their contribution to the deep radio, infrared, and X-ray counts, as well as to the diffuse extragalactic background radiation in these various spectral bands.

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