The Australia Telescope Large Area Survey: 2.3 GHz observations of ELAIS-S1 and CDF-S - Spectral index properties of the faint radio sky

@article{Zinn2012TheAT,
  title={The Australia Telescope Large Area Survey: 2.3 GHz observations of ELAIS-S1 and CDF-S - Spectral index properties of the faint radio sky},
  author={Peter Zinn and Enno Middelberg and Ray P. Norris and Christopher A. Hales and Minnie Y. Mao and Kate E. Randall},
  journal={Astronomy and Astrophysics},
  year={2012},
  volume={544},
  pages={1-11}
}
Context. The Australia Telescope Large Area Survey (ATLAS) aims to image a 7 deg 2 region centred on the European Large Area ISO Survey - South 1 (ELAIS-S1) field and the Chandra Deep Field South (CDF-S) at 1.4 GHz with high sensitivity (up to �∼ 10µJy) to study the evolution of star-forming galaxies (SFGs) and Active Galactic Nuclei (AGN) over a wide range of cosmic time. Aims. We present here ancillary radio observations at a frequency of 2.3 GHz obtained with the Australia Telescope Compact… Expand
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References

SHOWING 1-10 OF 62 REFERENCES
Deep Australia telescope large area survey radio observations of the European large area ISO survey S1/Spitzer wide-area infrared extragalactic field
We have conducted sensitive (1 σ < 30 μJy) 1.4 GHz radio observations with the Australia Telescope Compact Array of a field largely coincident with infrared observations of the Spitzer Wide-AreaExpand
Radio Observations of the Hubble Deep Field-South Region. III. The 2.5, 5.2, and 8.7 GHz Catalogs and Radio Source Properties
Deep radio observations of a wide region centered on the Hubble Deep Field-South have been performed, providing one of the most sensitive sets of radio observations acquired on the AustraliaExpand
Deep ATLAS radio observations of the CDFS-SWIRE field
We present the first results from the Australia Telescope Large Area Survey (ATLAS), which consist of deep radio observations of a 3.7 square degree field surrounding the Chandra Deep Field South,Expand
Deep ATLAS Radio Observations of the Chandra Deep Field-South/Spitzer Wide-Area Infrared Extragalactic Field
We present the first results from the Australia Telescope Large Area Survey, which consists of deep radio observations of a 3.7 deg2 field surrounding the Chandra Deep Field-South, largely coincidentExpand
THE VLA SURVEY OF CHANDRA DEEP FIELD SOUTH. V. EVOLUTION AND LUMINOSITY FUNCTIONS OF SUB-MILLIJANSKY RADIO SOURCES AND THE ISSUE OF RADIO EMISSION IN RADIO-QUIET ACTIVE GALACTIC NUCLEI
We present the evolutionary properties and luminosity functions of the radio sources belonging to the Chandra Deep Field South Very Large Array survey, which reaches a flux density limit at 1.4 GHzExpand
A search for distant radio galaxies from SUMSS and NVSS – III. Radio spectral energy distributions and the z–α correlation
This is the third in a series of papers that present observations and results for a sample of 76 ultrasteep-spectrum radio sources designed to find galaxies at high redshift. Here we presentExpand
The ATESP 5 GHz radio survey - I. Source counts and spectral index properties of the faint radio population
Context. The nature and evolutionary properties of the faint radio population, responsible for the steepening observed in the 1.4 GHz source counts below 1 milliJy, are not yet entirely clear. RadioExpand
THE DEEP SWIRE FIELD. I. 20 cm CONTINUUM RADIO OBSERVATIONS: A CROWDED SKY
We present results from deep radio observations taken with the Very Large Array at a center frequency of 1400 MHz covering a region of the Spitzer Wide-area InfraRed Extragalactic Survey of theExpand
MIPS 24 μm OBSERVATIONS OF THE HUBBLE DEEP FIELD SOUTH: PROBING THE IR-RADIO CORRELATION OF GALAXIES AT z>1
We present MIPS 24 μm observations of the Hubble Deep Field South taken with the Spitzer Space Telescope. The resulting image is 254 arcmin^2 in size and has a sensitivity ranging between ~12 andExpand
A search for distant radio galaxies from SUMSS and NVSS ¿ II. Optical spectroscopy
This is the second in a series of papers presenting observations and results for a sample of 76 ultra-steep-spectrum (USS) radio sources in the southern hemisphere designed to nd galaxies at highExpand
...
1
2
3
4
5
...