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WSRT 1.4 GHz Observations of the Hubble Deep Field

  • M.A. Garrett (a1), G. de Bruyn (a2), W. Baan (a1) and R.T. Schilizzi (a1)

Abstract

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.

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Copyright

References

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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.
Richards, E. A., Kellermann, K. I., Fomalont, E. B., Windhorst, R. A., Partridge, R. B. (1998) AJ , 116, 1039.

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