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The SCUBA-2 Large eXtragalactic Survey: 850 μm map, catalogue and the bright-end number counts of the XMM-LSS field

  • T. K. Garratt
  • , J. E. Geach
  • , Y. Tamura
  • , K. E.K. Coppin
  • , M. Franco
  • , Y. Ao
  • , C. C. Chen
  • , C. Cheng
  • , D. L. Clements
  • , Y. S. Dai
  • , H. Dannerbauer
  • , T. R. Greve
  • , B. Hatsukade
  • , H. S. Hwang
  • , L. Jiang
  • , K. Kohno
  • , M. P. Koprowski
  • , M. J. Michałowski
  • , M. Sawicki
  • , D. Scott
  • H. Shim, T. T. Takeuchi, W. H. Wang, Y. Q. Xue, C. Yang
  • UniversityofHertfordshire
  • Nagoya University
  • CAS - Purple Mountain Observatory
  • University of Science and Technology of China
  • Academia Sinica - Institute of Astronomy and Astrophysics
  • Chinese Academy of Sciences South America Center for Astronomy
  • Imperial College London
  • CAS - National Astronomical Observatories
  • Instituto de Astrofísica de Canarias
  • University of La Laguna
  • Technical University of Denmark
  • University College London
  • The University of Tokyo
  • Seoul National University
  • Peking University
  • Nicolaus Copernicus University in Toruń
  • Adam Mickiewicz University in Poznań
  • Saint Mary's University Halifax
  • University of British Columbia
  • Research Organization of Information and Systems, The Institute of Statistical Mathematics
  • Chalmers University of Technology

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

Abstract

We present 850 μm imaging of the XMM-LSS field observed for 170 h as part of the James Clerk Maxwell Telescope SCUBA-2 Large eXtragalactic Survey (S2LXS). S2LXS XMM-LSS maps an area of 9 deg2, reaching a moderate depth of 1σ 4 mJy beam−1. This is the largest contiguous area of extragalactic sky mapped by James Clerk Maxwell Telescope (JCMT) at 850 μm to date. The wide area of the S2LXS XMM-LSS survey allows us to probe the ultra-bright (S850μm 15 mJy), yet rare submillimetre population. We present the S2LXS XMM-LSS catalogue, which comprises 40 sources detected at >5σ significance, with deboosted flux densities in the range of 7–48 mJy. We robustly measure the bright-end of the 850 μm number counts at flux densities >7 mJy, reducing the Poisson errors compared to existing measurements. The S2LXS XMM-LSS observed number counts show the characteristic upturn at bright fluxes, expected to be motivated by local sources of submillimetre emission and high-redshift strongly lensed galaxies. We find that the observed 850 μm number counts are best reproduced by model predictions that include either strong lensing or source blending from a 15-arcsec beam, indicating that both may make an important contribution to the observed overabundance of bright single dish 850 μm selected sources. We make the S2LXS XMM-LSS 850 μm map and >5σ catalogue presented here publicly available.

Original languageEnglish
Pages (from-to)3669-3687
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume520
Issue number3
DOIs
StatePublished - 1 Apr 2023

Keywords

  • catalogues
  • galaxies: high-redshift
  • submillimetre: galaxies
  • surveys

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