J/MNRAS/409/L13     Herschel-SPIRE radio galaxies            (Chapman+, 2010)

Herschel-SPIRE, far-infrared properties of millimetre-bright and -faint radio galaxies. Chapman S.C., Ivison R.J., Roseboom I.G., Auld R., Bock J., Brisbin D., Burgarella D., Chanial P., Clements D.L., Cooray A., Eales S., Franceschini A., Giovannoli E., Glenn J., Griffin M., Mortier A.M.J., Oliver S.J., Omont A., Page M.J., Papageorgiou A., Pearson C.P., Perez-Fournon I., Pohlen M., Rawlings J.I., Raymond G., Rodighiero G., Rowan-Robinson M., Scott D., Seymour N., Smith A.J., Symeonidis M., Tugwell K.E., Vaccari M., Vieira J.D., Vigroux L., Wang L., Wright G. <Mon. Not. R. Astron. Soc., 409, L13-L18 (2010)> =2010MNRAS.409L..13C 2010MNRAS.409L..13C
ADC_Keywords: Galaxies, radio ; Millimetric/submm sources ; Redshifts Keywords: galaxies: evolution - galaxies: high-redshift - galaxies: starburst Abstract: 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 >1012L. 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. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tables1.dat 93 41 Properties of 20 submillimetre galaxies (SMGs) and 21 submillimetre-faint, optically faint radio galaxies (OFRGs) with detected SPIRE fluxes from the XID-24um sample -------------------------------------------------------------------------------- Byte-by-byte Description of file: tables1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Type [SO] SMG (submillimetre galaxy) or OFRG (optically faint radio galaxy) 3- 4 I2 h RAh Right ascension (J2000) (1) 6- 7 I2 min RAm Right ascension (J2000) (1) 9- 14 F6.3 s RAs Right ascension (J2000) (1) 16 A1 --- DE- Declination sign (J2000) (1) 17- 18 I2 deg DEd Declination (J2000) (1) 20- 21 I2 arcmin DEm Declination (J2000) (1) 23- 27 F5.2 arcsec DEs Declination (J2000) (1) 29- 35 A7 --- Name Name of source 38- 42 F5.3 --- zsp Spectroscopic redshift 45- 50 F6.1 uJy S1.4GHz Radio flux density at 1.4GHz 53- 57 F5.2 mJy S250 Herschel/SPIRE 250µm flux density 59- 64 F6.3 mJy S350 Herschel/SPIRE 350µm flux density 66- 71 F6.3 mJy S500 Herschel/SPIRE 500µm flux density 73- 76 F4.1 mJy S850 SCUBA 850µn flux density 78- 81 F4.2 arcsec Sep Distance of the SPIRE 250µm source from the 24µm centroid 83- 87 F5.2 Lsun LFIR Far-IR luminosity 89- 93 F5.2 K Tdust Dust temperature -------------------------------------------------------------------------------- Note (1): Spitzer-24µm positions -------------------------------------------------------------------------------- Acknowledgements: Scott Chapman, schapman(at)ast.cam.uk
(End) Patricia Vannier [CDS] 14-Apr-2011
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