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WSRT 1.4 GHz Observations of the Hubble Deep Field
Published online by Cambridge University Press: 26 May 2016
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
- Information
- Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 32 - 33
- 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)
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Richards, E. A., Kellermann, K. I., Fomalont, E. B., Windhorst, R. A., Partridge, R. B. (1998)
AJ
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