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

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posted on 2016-02-03, 11:42 authored by J. M. Simpson, I. Smail, A. M. Swinbank, S. C. Chapman, J. E. Geach, R. J. Ivison, A. P. Thomson, I. Aretxaga, Andrew William Blain, W. I. Cowley, C. -. C. Chen, K. E. K. Coppin, J. S. Dunlop, A. C. Edge, D. Farrah, E. Ibar, A. Karim, K. K. Knudsen, R. Meijerink, M. J. Michalowski, D. Scott, M. Spaans, P. P. van der Werf
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 ${S}_{\mathrm{SCUBA}-2}$ = 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 ${L}_{\mathrm{IR}}$ $\gtrsim $ 1012 ${\text{}}{L}_{\odot }$. 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 ${\text{}}{L}_{\odot }$ or a star formation rate (SFR) of ~103 ${\text{}}{M}_{\odot }\;{\mathrm{yr}}^{-1}$. For the typical sizes of these SMGs, which are resolved in our ALMA data with ${R}_{{\rm{e}}}$ = 1.2 ± 0.1 kpc, this yields a limiting SFR density of ~100 ${\text{}}{M}_{\odot }$ yr−1 kpc−2 Finally, the number density of S870 $\gtrsim $ 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.

History

Citation

Astrophysical Journal, 2015, 807 (2), 128

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Astrophysical Journal

Publisher

IOP Publishing LTD

issn

0004-637X

eissn

1538-4357

Acceptance date

2015-05-18

Copyright date

2015

Available date

2016-02-03

Publisher version

http://iopscience.iop.org/article/10.1088/0004-637X/807/2/128/meta

Language

en