Herschel-SPIRE radio galaxies (Chapman+, 2010)

Details Herschel-SPIRE radio galaxies (Chapman+, 2010) Herschel-SPIRE radio galaxies (Chapman+, 2010)

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74099013c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/409/L13. Originally published in: 2010MNRAS.409L..13C

Computer Science

Galaxies: Radio, Millimetric/Submm Sources, Redshifts

Scientific paper

We present the first study of the far-infrared (FIR) properties of high-redshift, radio-selected ultraluminous infrared galaxies (ULIRGs) using deep observations obtained with the Spectral and Photometric Imaging Receiver (SPIRE) from the Herschel Multi-tiered Extragalactic Survey (HerMES). These galaxies span a large range of 850-um fluxes from submillimetre-luminous ~10mJy sources (SCUBA galaxies) to ~1.5mJy from stacked SCUBA non-detections, thus likely representing a complete distribution of ULIRG spectral energy distributions (SEDs). From Keck spectroscopic surveys in the Lockman-North field we identified a sample of 31 submillimetre galaxies (SMGs) and 37 submillimetre-faint, optically faint radio galaxies (OFRGs), all with radio-inferred IR luminosities >1012^L&sun;. These galaxies were cross-identified with SPIRE 250-, 350- and 500-um catalogues based on fluxes extracted at 24-um positions in the SWIRE survey, yielding a sample of more than half of the galaxies well detected in at least two of the SPIRE bandpasses.
(1 data file).

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