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1998AJ....116.1039R - Astron. J., 116, 1039-1054 (1998/September-0)
Radio emission from galaxies in the Hubble Deep Field.
RICHARDS E.A., KELLERMANN K.I., FOMALONT E.B., WINDHORST R.A. and PARTRIDGE R.B.
Abstract (from CDS):
The microjansky radio sources are distributed over a wide range of redshifts (0.1 < z < 3) and have a typical monochromatic luminosity of about 1023 W.Hz–1. The majority of the optical identifications are with luminous (L > L*) galaxies at modest redshifts (0 ≲ z ≲ 1), many with evidence for recent star formation. The remainder are composed of a mixture of bright field elliptical galaxies and late-type galaxies with evidence of nuclear activity (LINERs and Seyfert galaxies) and nearby (z < 0.2) field spiral galaxies. None of the radio sources in this survey are identified with quasars or galactic stars.
Abstract Copyright: ∼
Journal keyword(s): Cosmology: Observations - Galaxies: Active - Galaxies: Evolution - Galaxies: Starburst - Radio Continuum
Nomenclature: Tables 3, 5: [RKF98] MMSS+MMSS N=41+19.
Simbad objects: 61
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