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

被引:7
|
作者
Garratt, T. K. [1 ]
Geach, J. E. [1 ]
Tamura, Y. [2 ]
Coppin, K. E. K. [1 ]
Franco, M. [1 ]
Ao, Y. [3 ,4 ]
Chen, C. -C [5 ]
Cheng, C. [6 ]
Clements, D. L. [7 ]
Dai, Y. S. [6 ,8 ]
Dannerbauer, H. [9 ,10 ]
Greve, T. R. [11 ,12 ]
Hatsukade, B. [13 ]
Hwang, H. S. [14 ,15 ]
Jiang, L. [16 ]
Kohno, K.
Koprowski, M. P. [17 ]
Michalowski, M. J. [18 ]
Sawicki, M. [19 ]
Scott, D. [20 ]
Shim, H. [21 ]
Takeuchi, T. T. [2 ,22 ]
Wang, W. -H [5 ]
Xue, Y. Q. [4 ,23 ]
Yang, C. [24 ]
机构
[1] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, England
[2] Nagoya Univ, Div Particle & Astrophys Sci, Nagoya, Aichi 4648602, Japan
[3] Chinese Acad Sci, Key Lab Radio Astron, Purple Mt Observ, 10 Yuanhua Rd, Nanjing 210023, Peoples R China
[4] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
[5] Acad Sinica, Sect 4, Inst Astron & Astrophys, 1 Roosevelt Rd, Taipei 10617, Taiwan
[6] Chinese Acad Sci, Natl Astron Observ, South Amer Ctr Astron, Beijing 100101, Peoples R China
[7] Imperial Coll London, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England
[8] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
[9] Inst Astrofis Canarias IAC, E-38205 Tenerife, Spain
[10] Univ Laguna, Dept Astrofis, E-38206 Tenerife, Spain
[11] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark
[12] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[13] Univ Tokyo, Inst Astron, Grad Sch Sci, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan
[14] Seoul Natl Univ, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea
[15] Seoul Natl Univ, SNU Astron Res Ctr, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea
[16] Peking Univ, Kavli Inst Astron & Astrophys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China
[17] Nicolaus Copernicus Univ, Inst Astron, Fac Phys, Astron & Informat, Grudziadzka 5, PL-87100 Torun, Poland
[18] Adam Mickiewicz Univ, Astron Observ Inst, Fac Phys, ul Sloneczna 36, PL-60286 Poznan, Poland
[19] St Marys Univ, Inst Computat Astrophys, Dept Astron & Phys, Halifax, NS B3H 3C3, Canada
[20] Univ British Columbia, Dept Phys & Astron, Vancouver, BC, Canada
[21] Kyungpook Natl Univ, Dept Earth Sci Educ, Daegu 41566, South Korea
[22] Inst Stat Math, Res Ctr Stat Machine Learning, 10-3 Midori Cho, Tachikawa, Tokyo 1908562, Japan
[23] Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
[24] Univ Technol, Dept Space Earth & Environm Chalmers, Gothenburg, Sweden
基金
英国科学技术设施理事会; 新加坡国家研究基金会; 国家重点研发计划; 加拿大创新基金会; 中国国家自然科学基金; 日本学术振兴会;
关键词
catalogues; surveys; galaxies:high; redshift; submillimetre:galaxies; COSMOLOGY LEGACY SURVEY; 850; MU-M; STAR-FORMING GALAXIES; DEEP SUBMILLIMETER SURVEY; FAR-INFRARED PROPERTIES; ACTIVE GALACTIC NUCLEI; POINT-SOURCE CATALOG; ALMA SURVEY; PHYSICAL-PROPERTIES; BOLOMETER CAMERA;
D O I
10.1093/mnras/stad307
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present 850 mu m 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 9deg(2) reaching a moderate depth of 1 sigma?4mJy beam(-1) 1J?4mJy beam(-1?). This is the largest contiguous area of extragalactic sky mapped by James Clerk Maxwell Telescope (JCMT) at 850 mu m to date. The wide area of the S2LXS XMM-LSS survey allows us to probe the ultra-bright (?S-850 mu m?15mJy ), yet rare submillimetre population. We present the S2LXS XMM-LSS catalogue, which comprises 40 sources detected at > 5 sigma significance, with deboosted flux densities in the range of 77-48mJy48mJy?. We robustly measure the bright-end of the 850 mu m number counts at flux densities > 7mJy > 7mJy?, 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 mu m 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 mu m selected sources. We make the S2LXS XMM-LSS 850 mu m map and > 5 sigma catalogue presented here publicly available.
引用
收藏
页码:3669 / 3687
页数:19
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