Submillimeter imaging of RCS J022434-0002.5: Intense activity in a high-redshift cluster?

被引:18
作者
Webb, TMA
Yee, HKC
Ivison, RJ
Hoekstra, H
Gladders, MD
Barrientos, LF
Hsieh, BC
机构
[1] Leiden Univ, Leiden Observ, NL-2333 CA Leiden, Netherlands
[2] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada
[3] Royal Observ, Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland
[4] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada
[5] Carnegie Observ, Pasadena, CA 91101 USA
[6] Pontificia Univ Catolica Chile, Fac Fis, Dept Astron & Astrofis, Santiago, Chile
[7] Natl Cent Univ, Astron Inst, Jhongli 320, Taoyuan County, Taiwan
[8] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan
关键词
dust; extinction; galaxies : clusters : individual (RCS J022434-0002.5); galaxies : evolution; galaxies : starburst; infrared : galaxies; radio continuum : galaxies;
D O I
10.1086/432524
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present deep 850 mu m imaging of the z = 0.773 strong lensing galaxy cluster RCS J022434-0002.5 from the Red-Sequence Cluster Survey (RCS). These data are part of a larger submillimeter survey of RCS clusters with SCUBA on the JCMT. We find five objects at 850 mu m, all of which are also detected at either 1.4 GHz or 450 mu m, or both. The number density of objects in this field is in general agreement with the blank-field source counts; however, when combined with other cluster surveys a general tendency of cluster fields toward higher submillimeter number densities is seen, which may be the result of unrecognized submillimeter luminous cluster galaxies. Primarily employing optical photometric redshifts, we show that two of the five submillimeter galaxies in this field are consistent with being cluster members, while two are more likely background systems.
引用
收藏
页码:187 / 196
页数:10
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