@article{73e6a38d40f44153ad03f39a824e91ce,
title = "Radio emission from objects in the hubble deep field",
abstract = "A radio image that covers the Hubble deep field and flanking fields has been made using the VLA for 50 hr at a frequency of 8.4 GHz, a resolution of 6″, and a 4.3 σ detection level of 12.2 μJy. All six radio sources detected in the deep field are identified with galaxies brighter than I = 24 mag, based on a radio/optical coincidence better than 1″. In the flanking fields 8 of 12 sources are identified with galaxies 19 to 25 mag. The identifications are preferentially with red elliptical galaxies and early-type spiral galaxies. Several galaxies show distortions that suggest interaction.",
keywords = "Galaxies: active, Radio continuum: galaxies",
author = "Fomalont, {E. B.} and Kellermann, {K. I.} and Richards, {E. A.} and Rogier Windhorst and Partridge, {R. B.}",
note = "Funding Information: This work was made possible through the foresight of R. Williams and the staff of the Space Telescope Science Institute in obtaining and making available the HDF images. We thank David Hogg, who provided the redshifts of galaxies in the HDF, and C. Steidel for providing his astrometric Palomar image. Part of this work was supported by NASA through grant AR-06337.02-94A from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-2655 and by a National Science Foundation grant AST-9320049 to Haverford College. E. A. R. acknowledges the support of a Sigma Xi grant-in-aid-of-research. The National Radio Astronomy Observatory is a facility of the National Science Foundation, which is operated by Associated Universities, Inc., under a cooperative agreement with the National Science Foundation.",
year = "1997",
doi = "10.1086/310457",
language = "English (US)",
volume = "475",
pages = "L5--L7",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "1 PART II",
}