Herschel Bright Sources (HerBS) Virtual Observatory Resource

Authors
  1. Bakx T.J.L.C.
  2. Eales S.A.
  3. Negrello M.
  4. Smith M.W.L.
  5. Valiante E.,Holland W.S.
  6. Baes M.
  7. Bourne N.
  8. Clements D.L.
  9. Dannerbauer H.,De Zotti G.
  10. Dunne L.
  11. Dye S.
  12. Furlanetto C.
  13. Ivison R.J.
  14. Maddox S.,Marchetti L.
  15. Michalowski M.J.
  16. Omont A.
  17. Oteo I.
  18. Wardlow J.L.,Van Der Werf P.
  19. Yang C.
  20. Published by
    CDS
Abstract

We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4deg^2^ Herschel Astrophysical Terahertz Large Area Survey. The HerBS sample contains 209 galaxies, selected with a 500um flux density greater than 80mJy and an estimated redshift greater than 2. The sample consists of a combination of hyperluminous infrared galaxies and lensed ultraluminous infrared galaxies during the epoch of peak cosmic star formation. In this paper, we present Submillimetre Common-User Bolometer Array 2 (SCUBA-2) observations at 850um of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) and 850um 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^+1.35^_-1.66_ and 45.80^+2.88^_-3.48_K, a cold-to-hot dust mass ratio of 26.62^+5.61^_-6.74_ and a {beta} of 1.83^+0.14^_-0.28_. Thee 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 are high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4+/-2.1 of those galaxies to be lensed (84.5 per cent). The SPIRE 500um flux suggests that out of all 209 HerBS sources, we expect 158.1+/-1.7 lensed sources, giving a total lensing fraction of 76 per cent.

Keywords
  1. galaxies
  2. infrared-sources
  3. millimeter-astronomy
  4. photometry
  5. submillimeter-astronomy
  6. redshifted
Bibliographic source Bibcode
2018MNRAS.473.1751B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/473/1751
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/473/1751
Document Object Identifer DOI
doi:10.26093/cds/vizier.74731751

Access

IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/473/1751/tablea1?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/473/1751/tablea1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/473/1751/tablea1?
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/473/1751/tablea2?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/473/1751/tablea2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/473/1751/tablea2?

History

2020-09-17T11:32:32Z
Resource record created
2020-09-17T11:32:32Z
Created
2024-08-17T20:21:22Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr