Submillimetre-wave surveys: first results and prospects

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dc.creatorBlain, Andrew W.
dc.date1998-06-29
dc.date1998-08-11
dc.date.accessioned2026-07-25T20:49:26Z
dc.descriptionThe population of distant dusty submm-luminous galaxies was first detected last year (Smail, Ivison and Blain 1997). Forms of evolution required to account for both this population and the intensity of background radiation have now been determined (Blain, Smail, Ivison and Kneib 1998), and are used to investigate the most efficient observing strategies for future surveys.
dc.description4 pages, 3 figures. Revised version includes updated references and details of the SCUBA upgrades programme
dc.identifierhttps://arxiv.org/abs/astro-ph/9806369
dc.identifierhttp://arxiv.org/abs/astro-ph/9806369
dc.identifierColombi S., Mellier Y. eds., `Wide Field surveys in cosmology', Editions Frontieres, p. 213-216
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/73449
dc.subjectAstrophysics
dc.titleSubmillimetre-wave surveys: first results and prospects
dc.typetext

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