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Search: onr:"swepub:oai:research.chalmers.se:c460ecc7-9dc5-47a6-a6e8-e1a826933089" > Meijerink R. > THE SCUBA-2 COSMOLO...

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THE SCUBA-2 COSMOLOGY LEGACY SURVEY: ALMA RESOLVES the BRIGHT-END of the SUB-MILLIMETER NUMBER COUNTS

Simpson, J. M. (author)
Durham University
Smail, I. (author)
Durham University
Swinbank, A.M. (author)
Durham University
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Chapman, S.C. (author)
Dalhousie University
Geach, J.E. (author)
University of Hertfordshire
Ivison, R.J. (author)
University of Edinburgh,European Southern Observatory (ESO)
Thomson, A. P. (author)
Durham University
Aretxaga, I. (author)
Instituto Nacional de Astrofísica, Óptica y Electrońica (INAOE),National Institute of Astrophysics, Optics and Electronics (INAOE)
Blain, A.W. (author)
University Of Leicester
Cowley, W.I. (author)
Durham University
Chen, C. C. (author)
Durham University
Coppin, K. E. K. (author)
University of Hertfordshire
Dunlop, J.S. (author)
University of Edinburgh
Edge, A. C. (author)
Durham University
Farrah, D. (author)
Virginia Polytechnic Institute and State University (Virginia Tech)
Ibar, E. (author)
Universidad de Valparaíso,University of Valparaíso
Karim, A. (author)
Universität Bonn,University of Bonn
Knudsen, Kirsten Kraiberg, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Meijerink, R. (author)
Universiteit Leiden (UL),Leiden University (UL)
Michalowski, M. J. (author)
University of Edinburgh
Scott, D. (author)
University of British Columbia (UBC)
Spaans, M. (author)
Rijksuniversiteit Groningen,University of Groningen
van der Werf, P.P. (author)
Universiteit Leiden (UL),Leiden University (UL)
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 (creator_code:org_t)
2015
2015
English.
In: Astrophysical Journal. - 1538-4357 .- 0004-637X. ; 807:2
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We present high-resolution 870 μm Atacama Large Millimeter/sub-millimeter Array (ALMA) continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1 degree2 850 μm maps from the SCUBA-2 Cosmology Legacy Survey, and are representative of the brightest sources in the field (median SSCUBA-2= 8.7 ± 0.4 mJy). We detect 52 sub-millimeter galaxies (SMGs) at >4σ significance in our 30 ALMA maps. In 61-15+19% of the ALMA maps the single-dish source comprises a blend of ≥2 SMGs, where the secondary SMGs are Ultra-luminous Infrared Galaxies (ULIRGs) with LIR ≳ 1012 L⊙. The brightest SMG contributes on average 80-2+6% of the single-dish flux density, and in the ALMA maps containing ≥2 SMGs the secondary SMG contributes 25-5+1% of the integrated ALMA flux. We construct source counts and show that multiplicity boosts the apparent single-dish cumulative counts by 20% at S870 > 7.5 mJy, and by 60% at S870 > 12 mJy. We combine our sample with previous ALMA studies of fainter SMGs and show that the counts are well-described by a double power law with a break at 8.5 ± 0.6 mJy. The break corresponds to a luminosity of ∼6 × 1012 L⊙ or a star formation rate (SFR) of ∼103 M⊙ yr-1. For the typical sizes of these SMGs, which are resolved in our ALMA data with Re = 1.2 ± 0.1 kpc, this yields a limiting SFR density of ∼100 M⊙ yr-1 kpc-2 Finally, the number density of S870 ≳ 2 mJy SMGs is 80 ± 30 times higher than that derived from blank-field counts. An over-abundance of faint SMGs is inconsistent with line-of-sight projections dominating multiplicity in the brightest SMGs, and indicates that a significant proportion of these high-redshift ULIRGs are likely to be physically associated.

Subject headings

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

Keyword

galaxies: starburst
submillimeter: galaxies
galaxies: abundances
galaxies: high-redshift
galaxies: star formation

Publication and Content Type

art (subject category)
ref (subject category)

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