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Exploring the infrared/radio correlation at high redshift

Abstract:: We have analysed the 24um properties of a radio-selected sample in the Subaru-XMM/Newton Deep Field in order to explore the behaviour of the FIR/radio relation at high redshifts. Statistically, the correlation is described by q24, the ratio between the observed flux densities at 24um and 1.4GHz, respectively. Using 24um data results in considerably more scatter in the correlation than previous work using data at 60-70um. Nevertheless, we do observe a steady correlation as a function of redshi...
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Publication status:: Published

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APA Style

Ibar, E., Cirasuolo, M., Ivison, R., Best, P., Smail, I., Biggs, A., Simpson, C., Dunlop, J., Almaini, O., McLure, R., Foucaud, S., & Rawlings, S. (2008). Exploring the infrared/radio correlation at high redshift. Monthly Notices of the Royal Astronomical Society, 386(2), 953–962.

MLA Style

Ibar, E., et al. “Exploring the Infrared/Radio Correlation at High Redshift.” Monthly Notices of the Royal Astronomical Society, vol. 386, no. 2, 2008, pp. 953–62.

Chicago Style

Ibar, E, M Cirasuolo, R Ivison, P Best, I Smail, A Biggs, C Simpson, et al. 2008. “Exploring the Infrared/Radio Correlation at High Redshift.” Monthly Notices of the Royal Astronomical Society 386 (2): 953–62.
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Publisher copy:: 10.1111/j.1365-2966.2008.13077.x

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+ Cirasuolo, M More by this author

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Bibliographic Details

Journal:: Monthly Notices of the Royal Astronomical Society
Volume:: 386
Issue:: 2
Pages:: 953-962
Publication date:: 2008-02-19
DOI:: 10.1111/j.1365-2966.2008.13077.x
EISSN:: 1365-2966
ISSN:: 0035-8711

Item Description

Keywords:: astro-ph
Pubs id:: pubs:23130
UUID:: uuid:cb87f7bd-b261-45f7-9d27-69968670d9b7
Local pid:: pubs:23130
Source identifiers:: 23130
Deposit date:: 2012-12-19

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Copyright date:: 2008
Notes:: The paper contains 7 figures and 1 table. In press at MNRAS

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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