Photometric Redshifts in the Hubble Deep Field

Details Photometric Redshifts in the Hubble Deep Field Photometric Redshifts in the Hubble Deep Field

1996-10-03

arxiv.org/abs/astro-ph/9610027v1

Astronomy and Astrophysics

Astrophysics

2 pages. To appear in the proceedings of the 37th Herstmonceux conference, "HST and the High Redshift Universe"

Scientific paper

Photometric redshifts for galaxies in the Hubble Deep Field are measured.
Luminosity functions show steepening of the faint-end slope and mild
brightening of M* out to z~3, followed by a decline at higher z; an excess of
faint, star-forming galaxies is seen at low z. Our results are consistent with
the formation of large galaxies at z=2-3, followed by that of dwarfs at z<1.

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