Open AccessThe SCUBA 8‐mJy survey – II. Multiwavelength analysis of bright submillimetre sources
Author(s) -
Fox M. J.,
Efstathiou A.,
RowanRobinson M.,
Dunlop J. S.,
Scott S.,
Serjeant S.,
Mann R. G.,
Oliver S.,
Ivison R. J.,
Blain A.,
Almaini O.,
Hughes D.,
Willott C. J.,
Longair M.,
Lawrence A.,
Peacock J. A.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05111.x
Subject(s) - physics , redshift , astrophysics , spectral energy distribution , galaxy , flux (metallurgy) , luminous infrared galaxy , millimeter , james clerk maxwell telescope , infrared , redshift survey , space observatory , astronomy , star formation , materials science , metallurgy
We present the results of a multiwavelength study of the 19 most significant submillimetre (submm) sources detected in the SCUBA 8‐mJy survey. As described in Scott et al., this survey covers ≃260 arcmin 2 using the submillimetre camera SCUBA, to a limiting source detection limit S 850 μm ≃8 mJy . One advantage of this relatively bright flux‐density limit is that accurate astrometric positions are potentially achievable for every source using existing radio and/or millimetre‐wave interferometers. However, an associated advantage is that spectral energy distribution (SED) based redshift constraints should be more powerful than in fainter submm surveys. Here we therefore exploit the parallel SCUBA 450‐μm data, in combination with existing radio and Infrared Space Observatory ( ISO ) data at longer and shorter wavelengths to set constraints on the redshift of each source. We also analyse new and existing optical and near‐infrared imaging of our SCUBA survey fields to select potential identifications consistent with these constraints. Our derived SED‐based redshift constraints, and the lack of statistically significant associations with even moderately bright galaxies allow us to conclude that all 19 sources lie at z >1 , and at least half of them apparently lie at z >2 .