作者: James Higdon , Minh T. Huynh , Mark H. Wieringa , Brian J. Boyle , Daniel A. Mitchell
DOI: 10.1086/432872
关键词: Quasar 、 Radio galaxy 、 Galaxy 、 Luminous infrared galaxy 、 Hubble Deep Field South 、 Hubble Deep Field 、 Hubble Ultra-Deep Field 、 Redshift 、 Astronomy 、 Physics 、 Astrophysics
摘要: This paper is the first of a series describing results Australia Telescope Hubble Deep Field–South radio survey. The survey was conducted at four wavelengths, 20, 11, 6, and 3 cm, over 4 year period achieves an rms sensitivity about 10 μJy each wavelength. We describe observations data reduction processes present on sources close to center Field–South. discuss in detail properties subset these sources. include both starburst galaxies powered by active galactic nucleus range redshift from 0.1 2.2. Some them are characterized unusually high radio-to-optical luminosities, presumably caused dust extinction.