Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-05-11
Astron.J.130:1358-1372,2005
Astronomy and Astrophysics
Astrophysics
Accepted by AJ. 32 pages, 4 tables, 3 figures. PDF with full-resolution figures is on http://www.atnf.csiro.au/people/rnorri
Scientific paper
10.1086/432872
This paper is the first of a series describing the results of the Australia Telescope Hubble Deep Field South (ATHDFS) radio survey. The survey was conducted at four wavelengths - 20, 11, 6, and 3 cm, over a 4-year period, and achieves an rms sensitivity of about 10 microJy at each wavelength. We describe the observations and data reduction processes, and present data on radio sources close to the centre of the HDF-S. We discuss in detail the properties of a subset of these sources. The sources include both starburst galaxies and galaxies powered by an active galactic nucleus, and range in redshift from 0.1 to 2.2. Some of them are characterised by unusually high radio-to-optical luminosities, presumably caused by dust extinction.
Boyle Brian J.
Ekers Ronald D.
Higdon James J.
Hopkins Andrew M.
Huynh Minh T.
No associations
LandOfFree
Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-73983