Submillimetre detection of the z = 2.83 Lyman-break galaxy, Westphal-MM8, and implications for SCUBA2

被引:23
作者
Chapman, S. C. [1 ,2 ]
Casey, C. M. [1 ]
机构
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
galaxies: active; galaxies: formation; galaxies: individual: Westphal-MM8; infrared: galaxies; DEGREE EXTRAGALACTIC SURVEY; HUBBLE-DEEP-FIELD; ULTRAVIOLET LUMINOSITY DENSITY; CLERK-MAXWELL-TELESCOPE; STAR-FORMATION HISTORY; STARBURST GALAXIES; HIGH-REDSHIFT; INFRARED GALAXIES; MOLECULAR GAS; POPULATION;
D O I
10.1111/j.1365-2966.2009.14710.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present confusion-limited submillimetre (submm) observations with the Submillimetre Common-User Bolometer Array (SCUBA) camera on the James Clerk Maxwell Telescope of the z = 2.83 Lyman-break galaxy (LBG), Westphal-MM8, reaching an 850 mu m sensitivity even greater than that achieved in the SCUBA map of the Hubble Deep Field region. The detection of MM8 (S(850 mu m) = 1.98 +/- 0.48 mJy), along with the literature submm detections of lensed LBGs, suggests that the LBG population may contribute significantly to the source counts of submm-selected galaxies in the 1-2 mJy regime. Additionally, submm-luminous LBGs are a viable progenitor population for the recently discovered evolved galaxies at z similar to 2-2.5. These observations represent an important baseline for SCUBA2 observations which will regularly map large regions of the sky to this depth.
引用
收藏
页码:1615 / 1620
页数:6
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