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Sub-millimetre source identifications and the micro-Jansky source population at 8.4 GHz in the William Herschel Deep Field

Abstract:

[Abridged] Sub-mm observations of the William Herschel Deep Field using LABOCA revealed possible counterparts for 2 X-ray absorbed QSOs. The aim here is to exploit EVLA imaging at 8.4 GHz to establish the QSOs as radio/sub-mm sources. The challenge in reducing the EVLA data was the presence of a strong 4C source in the field. A new calibration algorithm was applied to the data to subtract it. The resulting thermal noise limited radio map covers the 16'x16' Extended WHDF. It contains 41 source...

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Publication status:
Published

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Publisher copy:
10.1093/mnras/sts046

Authors


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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Bielby, RM More by this author
Metcalfe, N More by this author
Rawlings, S More by this author
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Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
428
Issue:
2
Pages:
935-951
Publication date:
2012-09-20
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:ceccf755-9be0-4edc-8447-ecbc57623ab0
Source identifiers:
388280
Local pid:
pubs:388280
Language:
English
Keywords:

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