| dc.contributor.author | Borys, Colin | en_US |
| dc.contributor.author | Chapman, Scott | en_US |
| dc.contributor.author | Halpern, Mark | en_US |
| dc.contributor.author | Scott, Douglas | en_US |
| dc.date.accessioned | 2014-03-12T19:21:05Z | |
| dc.date.available | 2014-03-12T19:21:05Z | |
| dc.date.issued | 2002-03 | en_US |
| dc.identifier.citation | Borys, Colin, Scott Chapman, Mark Halpern, and Douglas Scott. 2002. "A SCUBA Scanmap of the HDF: Measuring the bright end of the sub-mm source counts." Monthly Notices of the Royal Astronomical Society 330(3): 63-L67 | en_US |
| dc.identifier.issn | 0035-8711 | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1046/j.1365-8711.2002.05347.x | en_US |
| dc.identifier.uri | http://hdl.handle.net/10222/45478 | |
| dc.description.abstract | Using the 850 micron SCUBA camera on the JCMT and a scanning technique different from other sub-mm surveys, we have obtained a 125 square arcminute map centered on the Hubble Deep Field. The one-sigma sensitivity to point sources is roughly 3 mJy and thus our map probes the brighter end of the sub-mm source counts. We find 6 sources with a flux greater than about 12 mJy (>4 sigma) and, after a careful accounting of incompleteness and flux bias, estimate the integrated density of bright sources N(>12 mJy)= 164 (+77/-58) per square degree (68 per cent confidence bounds). | en_US |
| dc.title | A SCUBA Scanmap of the Hubble Deep Field: Measuring the bright end of the sub-mm source counts | en_US |
| dc.title.alternative | Monthly Notices of the Royal Astronomical Society | en_US |
| dc.type | article | en_US |
| dc.identifier.volume | 330 | en_US |
| dc.identifier.issue | 3 | en_US |
| dc.identifier.startpage | 63 | en_US |
