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The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations

Authors :
Bakx, Tom J. L. C.
Eales, S. A.
Negrello, M.
Smith, M. W. L.
Valiante, E.
Holland, W. S.
Baes, M.
Bourne, N.
Clements, D. L.
Dannerbauer, H.
De Zotti, G.
Dunne, L.
Dye, S.
Furlanetto, C.
Ivison, R. J.
Maddox, S.
Marchetti, L.
Michałowski, M. J.
Omont, A.
Oteo, I.
Wardlow, J. L.
van der Werf, P.
Yang, C.
Bakx, Tom J. L. C.
Eales, S. A.
Negrello, M.
Smith, M. W. L.
Valiante, E.
Holland, W. S.
Baes, M.
Bourne, N.
Clements, D. L.
Dannerbauer, H.
De Zotti, G.
Dunne, L.
Dye, S.
Furlanetto, C.
Ivison, R. J.
Maddox, S.
Marchetti, L.
Michałowski, M. J.
Omont, A.
Oteo, I.
Wardlow, J. L.
van der Werf, P.
Yang, C.
Publication Year :
2017

Abstract

We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample contains 209 galaxies, selected with a 500 {\mu}m flux density greater than 80 mJy and an estimated redshift greater than 2. The sample consists of a combination of HyLIRGs and lensed ULIRGs during the epoch of peak cosmic star formation. In this paper, we present SCUBA-2 observations at 850 ${\mu}$m of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-SPIRE and 850 ${\mu}$m SCUBA-2 flux densities of 22 sources with spectroscopically determined redshifts, using a two-component modified blackbody spectrum as a template. We find a cold- and hot-dust temperature of 21.29 K and 45.80 K, a cold-to-hot dust mass ratio of 26.62 and a $\beta$ of 1.83. The poor quality of the fit suggests that the sample of galaxies is too diverse to be explained by our simple model. Comparison of our sample to a galaxy evolution model indicates that the fraction of lenses is high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4 $\pm$ 2.1 of those galaxies to be lensed (84.5%). The SPIRE 500 ${\mu}$m flux suggests that out of all 209 HerBS sources, we expect 158.1 $\pm$ 1.7 lensed sources, giving a total lensing fraction of 76 per cent.

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1363483953
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1093.mnras.stx2267