Radio observations of the Hubble Deep Field-South region. I. Survey description and initial results

被引：15
|
作者：
Norris, RP
Huynh, MT
Jackson, CA
Boyle, BJ
Ekers, RD
Mitchell, DA
Sault, RJ
Wieringa, MH
Williams, RE
Hopkins, AM
Higdon, J
机构：
[1] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[2] Australian Natl Univ, Mt Stromlo Observ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[4] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[5] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
来源：
ASTRONOMICAL JOURNAL | 2005年 / 130卷 / 04期
关键词：
quasars : general; radio continuum : galaxies; surveys;
D O I：
10.1086/432872
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This paper is the first of a series describing the results of the Australia Telescope Hubble Deep Field-South 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 mu Jy at each wavelength. We describe the observations and data reduction processes and present data on radio sources close to the center of the Hubble Deep Field-South. 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 characterized by unusually high radio-to-optical luminosities, presumably caused by dust extinction.
引用
收藏
页码：1358 / 1372
页数：15
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