White, Glenn J.; Hatsukade, Bunyo; Pearson, Chris; Takagi, Toshinobu; Sedgwick, Chris; Matsuura, Shuji; Matsuhara, Hideo; Serjeant, Stephen; Nakagawa, Takao; Lee, Hyung Mok; Oyabu, Shinki; Jeong, Woong-Seob; Shirahata, Mai; Kohno, Kotaro; Yammamura, Issei; Hanami, Hitoshi; Goto, Tomotsugu; Makiuti, Sin'itirou; Clements, David L.; Malek, K. and Khan, Sophia A.
PDF (Accepted Manuscript)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (1510Kb) | Preview
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1111/j.1365-2966.2012.21684.x|
|Google Scholar:||Look up in Google Scholar|
The results of a deep 20 cm radio survey at 20 cm are reported of the AKARI Deep Field South (ADF-S) near the South Ecliptic Pole (SEP), using the Australia Telescope Compact Array telescope, ATCA. The survey has 1σ detection limits ranging from 18.7--50 μJy per beam-1 over an area of ~1.1 degree2, and ~2.5 degree2 to lower sensitivity. The observations, data reduction and source count analysis are presented, along with a description of the overall scientific objectives, and a catalogue containing 530 radio sources detected with a resolution of 6.2" x 4.9". The derived differential source counts show a pronounced excess of sources fainter than ~1 mJy, consistent with an emerging population of star forming galaxies. Cross-correlating the radio with AKARI sources and archival data we find 95 cross matches, with most galaxies having optical R-magnitudes in the range 18-24 magnitudes, and 52 components lying within 1" of a radio position in at least one further catalogue (either IR or optical). We have reported redshifts for a sub-sample of our catalogue finding that they vary between galaxies in the local universe to those having redshifts of up to 0.825. Associating the radio sources with the Spitzer catalogue at 24 μm, we find 173 matches within one Spitzer pixel, of which a small sample of the identifications are clearly radio loud compared to the bulk of the galaxies. The radio luminosity plot and a colour-colour analysis suggest that the majority of the radio sources are in fact luminous star forming galaxies, rather than radio-loud AGN. There are additionally five cross matches between ASTE or BLAST submillimetre galaxies and radio sources from this survey, two of which are also detected at 90 μm, and 41 cross-matches with submillimetre sources detected in the Herschel HerMES survey Public Data release.
|Item Type:||Journal Article|
|Copyright Holders:||2012 The Authors|
|Keywords:||astrophysics; cosmology; extragalactic astrophysics|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||20 Nov 2012 10:15|
|Last Modified:||07 Oct 2016 03:20|
|Share this page:|
Download history for this item
These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.