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WSRT 1.4 GHz Observations of the Hubble Deep Field

Published online by Cambridge University Press:  26 May 2016

M.A. Garrett
Affiliation:
JIVE, Postbus 2, 7990 AA, Dwingeloo, NL
G. de Bruyn
Affiliation:
NFRA, Postbus 2, 7990 AA, Dwingeloo, NL
W. Baan
Affiliation:
JIVE, Postbus 2, 7990 AA, Dwingeloo, NL
R.T. Schilizzi
Affiliation:
JIVE, Postbus 2, 7990 AA, Dwingeloo, NL

Abstract

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We present WSRT 1.38 GHz observations of the Hubble Deep Field (and flanking fields). 72 hours of data were combined to produce the WSRT's deepest image yet, reaching an r.m.s. noise level of 8 microJy/beam. We detect radio emission from galaxies both in the HDF and HFF which have not been previously detected by recent MERLIN or VLA studies of the field.

Type
Part 1: Radio Source Surveys and Cosmology
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Muxlow, T.W.B., Wilkinson, P.N., Richards, A.M.S., Kellerman, K.I., Richards, E.A., Garrett, M.A. (1999) New Astronomy Reviews , 43, 623.CrossRefGoogle Scholar
Richards, E. A., Kellermann, K. I., Fomalont, E. B., Windhorst, R. A., Partridge, R. B. (1998) AJ , 116, 1039.Google Scholar