Journal article

A submillimetre survey of the star-formation history of radio galaxies

Abstract:: We present the results of the first major systematic submillimetre survey of radio galaxies spanning the redshift range 1 < z < 5. The primary aim of this work is to elucidate the star-formation history of this sub-class of elliptical galaxies by tracing the cosmological evolution of dust mass. Using SCUBA on the JCMT we have obtained 850-micron photometry of 47 radio galaxies to a consistent rms depth of 1 mJy, and have detected dust emission in 14 cases. The radio galaxy targets have ...
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APA Style

Archibald, E., Dunlop, J., Hughes, D., Rawlings, S., Eales, S. A., & Ivison, R. (2000). A submillimetre survey of the star-formation history of radio galaxies. Monthly Notices of the Royal Astronomical Society, 323(2), 417.

MLA Style

Archibald, E., et al. “A Submillimetre Survey of the Star-Formation History of Radio Galaxies.” Monthly Notices of the Royal Astronomical Society, vol. 323, no. 2, 2000, p. 417.

Chicago Style

Archibald, E, J Dunlop, D Hughes, S Rawlings, SA Eales, and R Ivison. 2000. “A Submillimetre Survey of the Star-Formation History of Radio Galaxies.” Monthly Notices of the Royal Astronomical Society 323 (2): 417.
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Publisher copy:: 10.1046/j.1365-8711.2001.04188.x

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+ Archibald, E More by this author

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+ Dunlop, J More by this author

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+ Hughes, D More by this author

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+ Rawlings, S More by this author

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+ Eales, SA More by this author

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Bibliographic Details

Journal:: Monthly Notices of the Royal Astronomical Society More from this journal
Volume:: 323
Issue:: 2
Pages:: 417
Publication date:: 2000-02-03
DOI:: 10.1046/j.1365-8711.2001.04188.x
EISSN:: 1365-2966
ISSN:: 0035-8711

Item Description

Keywords:: astro-ph
Pubs id:: pubs:1479
UUID:: uuid:6f93459a-0e41-4927-aa8b-2cf3b465b248
Local pid:: pubs:1479
Source identifiers:: 1479
Deposit date:: 2012-12-19

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Copyright date:: 2000
Notes:: 31 pages - 10 figures in main text, 3 pages of figures in appendix.
This revised version has been re-structured, but the analysis and conclusions
have not changed. Accepted for publication in MNRAS

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

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