Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution - CNRS - Centre national de la recherche scientifique Accéder directement au contenu
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2012

Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution

D. A. Riechers
  • Fonction : Auteur
A. Karim
  • Fonction : Auteur
P. Capak
M. Elvis
  • Fonction : Auteur
J. Kartaltepe
S. Lilly
  • Fonction : Auteur
D. Sanders
Y. Taniguchi
  • Fonction : Auteur
V. Smolcic
  • Fonction : Auteur
M. Aravena
F. Navarrete
  • Fonction : Auteur
E. Schinnerer

Résumé

We present new IRAM Plateau de Bure interferometer (PdBI) 1.3 mm continuum observations at similar to 1.5 `' resolution of 28 submillimeter galaxies (SMGs), previously discovered with the 870 mu m bolometer LABOCA at the APEX telescope from the central 0.7 deg(2) of the COSMOS field. Nineteen out of the 28 LABOCA sources were detected with PdBI at a greater than or similar to 3 sigma level of approximate to 1.4 mJy/beam. A combined analysis of this new sample with existing interferometrically identified SMGs in the COSMOS field yields the following results: i) greater than or similar to 15%, and possibly up to similar to 40% of single-dish detected SMGs consist of multiple sources; ii) statistical analysis of multi-wavelength counterparts to single-dish SMGs shows that only similar to 50% have real radio or IR counterparts; iii) similar to 18% of interferometric SMGs have either no multi-wavelength counterpart or only a radio-counterpart; and iv) similar to 50-70% of z greater than or similar to 3 SMGs have no radio counterparts (down to an rms of 7-12 mu Jy at 1.4 GHz). Using the exact interferometric positions to identify the multi-wavelength counterparts allows us to determine accurate photometric redshifts for these sources. The redshift distributions of the combined and the individual 1.1 mm and 870 mu m selected samples shows a higher mean and a broader width than those derived in previous studies. This study finds that on average brighter and/or mm-selected SMGs are located at higher redshifts, consistent with previous studies. The mean redshift for the 1.1 mm selected sample ((z) over bar = 3.1 +/- 0.4) is tentatively higher than that for the 870 mu m selected sample ((z) over bar = 2.6 +/- 0.4). Based on our nearly complete sample of AzTEC 1.1 mm SMGs in a 0.15 deg(2) area, we infer a higher surface density of z greater than or similar to 4 SMGs than predicted by current cosmological models. In summary, our findings imply that interferometric identifications at (sub-) millimeter wavelengths are crucial to build statistically complete and unbiased samples of SMGs.

Dates et versions

hal-01442378 , version 1 (20-01-2017)

Identifiants

Citer

D. A. Riechers, F. Bertoldi, C. Feruglio, A. Finoguenov, M. Salvato, et al.. Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution. Astronomy and Astrophysics - A&A, 2012, 548, ⟨10.1051/0004-6361/201219368⟩. ⟨hal-01442378⟩
107 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More