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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3938

Title: ATLBS: the Australia telescope low-brightness survey
Authors: Subrahmanyan, Ravi
Ekers, R.D.
Saripalli, Lakshmi
Sadler, E.M.
Keywords: echniques: interferometric
galaxies: active
galaxies: evolution
high-redshift
nuclei radio continuum:
Issue Date: 11-Jan-2010
Publisher: Wiley Interscience for the RAS
Citation: Monthly Notices of the Royal Astronomical Society, 2010, Vol.402, p2792
Abstract: We present a radio survey carried out with the Australia Telescope Compact Array. A motivation for the survey was to make a complete inventory of the diffuse emission components as a step towards a study of the cosmic evolution in radio source structure and the contribution from radio-mode feedback on galaxy evolution. The Australia Telescope Low-Brightness Survey (ATLBS) at 1388 MHz covers 8.42 deg2 of the sky in an observing mode designed to yield images with exceptional surface brightness sensitivity and low confusion. The survey was carried out in two adjacent regions on the sky centred at RA: 00h35m00s , Dec.: and RA: 00h59m17s , Dec.: (J2000.0). The ATLBS radio images, made with 0.08 mJy beam−1 rms noise and 50 arcsec beam, detect a total of 1094 sources with peak flux exceeding 0.4 mJy beam−1. The ATLBS source counts were corrected for blending, noise bias, resolution and primary beam attenuation; the normalized differential source counts are consistent with no upturn down to 0.6 mJy. The percentage integrated polarization Π0 was computed after corrections for the polarization bias in integrated polarized intensity; Π0 shows an increasing trend with decreasing flux density. Simultaneous visibility measurements made with longer baselines yielded images, with 5 arcsec beam, of compact components in sources detected in the survey. The observations provide a measurement of the complexity and diffuse emission associated with mJy and sub-mJy radio sources. 10 per cent of the ATLBS sources have more than half of their flux density in extended emission and the fractional flux in diffuse components does not appear to vary with flux density, although the percentage of sources that have complex structure increases with flux density. The observations are consistent with a transition in the nature of extended radio sources from FR-ii radio source morphology, which dominates the mJy population, to FR-i structure at sub-mJy flux density.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/3938
ISSN: 1365-2966 (Online)
0035-8711
Alternative Location: http://adsabs.harvard.edu/abs/2010MNRAS.402.2792S
http://arxiv.org/abs/0911.4571
http://dx.doi.org/10.1111/j.1365-2966.2009.16105.x
Copyright: 2010 The authors & the Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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