The Brighter Side of Sub-Mm Source Counts:. a SCUBA Scan-Map of the Hubble Deep Field

Details The Brighter Side of Sub-Mm Source Counts:. a SCUBA Scan-Map of the Hubble Deep Field The Brighter Side of Sub-Mm Source Counts:. a SCUBA Scan-Map of the Hubble Deep Field

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001dms..conf...93b&link_type=abstract

DEEP MILLIMETER SURVEYS Implications for Galaxy Formation and Evolution. Held 19-21 June 2000 in University of Massachusetts, Am

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We present an 11 × 11 sq. arcmin map centred on the Hubble Deep Field taken at 850 μm with the SCUBA camera on the JCMT. The map has an average one-sigma sensitivity to point sources of about 2.3 mJy and thus probes the brighter end of the sub-mm source counts. We find 7 sources with a flux greater than 9mJy ( 4σ), and therefore estimate N(> 9 mJy) = 208-72+90 degree-1. This result is consistent with work from other groups, but improves the statistics at the bright end, and is suggestive of a steepening of the counts.

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