Astronomy and Astrophysics – Astronomy
Scientific paper
May 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..685e&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, May 1983, p. 685-693. Research supported by the Sc
Astronomy and Astrophysics
Astronomy
21
Galactic Evolution, Galaxies, Infrared Astronomy, Red Shift, Color, Infrared Spectrophotometers, Star Formation Rate
Scientific paper
The infrared color-redshift relation for galaxies of known redshift is reexamined. The relation defined by measurements of optically selected galaxies lies fairly close to that expected from model predictions. Infrared colors may therefore offer a reasonable method for separating the effects of luminosity evolution and redshift when discussing optically selected samples of faint field galaxies. This method is applied to a complete sample of 47 field galaxies at optical magnitude 21.5. The infrared and optical data imply that a third of the field galaxies lie at redshifts beyond those expected from nonevolution models. The optical-to-infrared colors of these distant galaxies are generally bluer and the entire sample is consistent with a more vigorous star formation rate beyond a redshift of about 0.5.
Allen David A.
Ellis Richard S.
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