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Submillimetre sources in rich cluster fields - source counts, redshift estimates, and cooling flow limits

dc.contributor.authorChapman, Scott C.en_US
dc.contributor.authorScott, Douglasen_US
dc.contributor.authorBorys, Colinen_US
dc.contributor.authorFahlman, Gregory G.en_US
dc.date.accessioned2014-03-12T19:21:08Z
dc.date.available2014-03-12T19:21:08Z
dc.date.issued2002-02-11en_US
dc.description.abstractRecent submillimetre surveys have revealed a population of dusty, high redshift sources of great cosmological significance for understanding dust-enshrouded star formation in distant galaxies, and for determining the origin of the far-IR background. In this paper, we analyze nine rich cluster fields mapped at 850 and 450 microns with the SCUBA array on the James Clerk Maxwell telescope. Lensing models of the clusters are developed in order to derive accurate source counts for our sample. VLA maps of the same clusters are used to help constrain the redshift distribution of our SCUBA detections. Implications for high redshift galaxies and for the far-IR background are discussed. We also provide limits on distributed dust produced by cooling flows in these clusters.en_US
dc.identifier.citationChapman, Scott C., Douglas Scott, Colin Borys, and Gregory G. Fahlman. 2002. "Submillimetre sources in rich cluster fields - source counts, redshift estimates, and cooling flow limits." Monthly Notices of the Royal Astronomical Society 330(1): 92-104en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issue1en_US
dc.identifier.startpage92en_US
dc.identifier.urihttp://dx.doi.org/10.1046/j.1365-8711.2002.05053.xen_US
dc.identifier.urihttp://hdl.handle.net/10222/45546
dc.identifier.volume330en_US
dc.titleSubmillimetre sources in rich cluster fields - source counts, redshift estimates, and cooling flow limitsen_US
dc.title.alternativeMonthly Notices of the Royal Astronomical Societyen_US
dc.typearticleen_US

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