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The LABOCA survey of the Extended Chandra Deep Field-South: a photometric redshift survey of submillimetre galaxies

Wardlow, J. L. (author)
University of California at Irvine (UCI),Durham University
Smail, I. (author)
Durham University
Coppin, K. E. K. (author)
Durham University
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Alexander, D. M. (author)
University of California at Irvine (UCI)
Brandt, W. N. (author)
Pennsylvania State University
Danielson, A. L. R. (author)
University of California at Irvine (UCI)
Luo, B. (author)
Pennsylvania State University
Swinbank, A. M. (author)
Durham University
Walter, F. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Weiss, A. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Xue, Y. Q. (author)
Pennsylvania State University
Zibetti, S. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Bertoldi, F. (author)
Biggs, A. D. (author)
European Southern Observatory (ESO)
Chapman, S. C. (author)
University Of Cambridge
Dannerbauer, H. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Dunlop, J.S. (author)
University of Edinburgh
Gawiser, E. (author)
Rutgers University
Ivison, R. J. (author)
University of Edinburgh,Royal Observatory
Knudsen, Kirsten Kraiberg, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Kovacs, A. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Lacey, C. G. (author)
Durham University
Menten, K. M. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Padilla, N. (author)
Pontificia Universidad Catolica de Chile
Rix, H. W. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
van der Werf, P.P. (author)
Universiteit Leiden (UL),Leiden University (UL)
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 (creator_code:org_t)
2011-06-16
2011
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 415:2, s. 1479-1508
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We derive photometric redshifts from 17-band optical to mid-infrared photometry of 78 robust radio, 24-mu m and Spitzer IRAC counterparts to 72 of the 126 submillimetre galaxies (SMGs) selected at 870 mu m by LABOCA observations in the Extended Chandra Deep Field-South (ECDF-S). We test the photometric redshifts of the SMGs against the extensive archival spectroscopy in the ECDF-S. The median photometric redshift of identified SMGs is z = 2.2 +/- 0.1, the standard deviation is sigma(z) = 0.9 and we identify 11 (similar to 15 per cent) high-redshift (z >= 3) SMGs. A statistical analysis of sources in the error circles of unidentified SMGs identifies a population of possible counterparts with a redshift distribution peaking at z = 2.5 +/- 0.2, which likely comprises similar to 60 per cent of the unidentified SMGs. This confirms that the bulk of the undetected SMGs are coeval with those detected in the radio/mid-infrared. We conclude that at most similar to 15 per cent of all the SMGs are below the flux limits of our IRAC observations and thus may lie at z greater than or similar to 3 and hence at most similar to 30 per cent of all SMGs have z greater than or similar to 3. We estimate that the full S(870 mu m) > 4mJy SMG population has a median redshift of 2.5 +/- 0.5. In contrast to previous suggestions, we find no significant correlation between submillimetre flux and redshift. The median stellar mass of the SMGs derived from spectral energy distribution fitting is (9.1 +/- 0.5) x 10(10)M(circle dot) although we caution that the uncertainty in the star formation histories results in a factor of similar to 5 uncertainty in these stellarmasses. Using a single temperature modified blackbody fit with beta = 1.5, the median characteristic dust temperature of SMGs is 37.4 +/- 1.4K. The infrared luminosity function shows that SMGs at z = 2-3 typically have higher far-infrared luminosities and luminosity density than those at z = 1-2. This is mirrored in the evolution of the star formation rate density (SFRD) for SMGs which peaks at z similar to 2. The maximum contribution of bright SMGs to the global SFRD (similar to 5 per cent for SMGs with S(870 mu m) greater than or similar to 4mJy or similar to 50 per cent extrapolated to SMGs with S(870 mu m) > 1mJy) also occurs at z similar to 2.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

spitzer-space-telescope
galaxies: starburst
mu-m observations
degree extragalactic survey
function
sources
v614
star-forming galaxies
yale-chile musyc
submillimetre: galaxies
carthy pj
similar-to 2.5
luminous infrared galaxies
galaxies: evolution
scuba super-map
2004
galaxies: high-redshift
p9
x-ray
initial mass

Publication and Content Type

art (subject category)
ref (subject category)

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