WSRT 1.4 GHz Observations of the Hubble Deep Field
Astrophysics
2007-05-23 v1
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, achieving an r.m.s. noise level of 8 microJy per 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.
Keywords
Cite
@article{arxiv.astro-ph/0001523,
title = {WSRT 1.4 GHz Observations of the Hubble Deep Field},
author = {M. A. Garrett and G. de Bruyn and W. Baan and R. T. Schilizzi},
journal= {arXiv preprint arXiv:astro-ph/0001523},
year = {2007}
}
Comments
2 pages, 1 figure, to appear in "The Universe at Low Radio Frequencies", IAU Symposium 199. For colour figures, see http://www.nfra.nl/~mag/hdf_wsrt.html