Extending the redshift distribution of submm galaxies:: Identification of a z ≈ 4 submm galaxy

被引：0

作者：

Knudsen, K. K. ^{[1
]}

Kneib, J. -P. ^{[2
,3
]}

Egami, E. ^{[4
]}

机构：

[1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[2] OAMP, Lab Astrophys Marseille, F-13012 Marseille, France

[3] CALTECH, Pasadena, CA 91125 USA

[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

来源：

SECOND ANNUAL SPITZER SCIENCE CENTER CONFERENCE: INFRARED DIAGNOSTICS OF GALAXY EVOLUTION | 2008年 / 381卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the identification of a bright submillimeter galaxy (SMG) in the field of Abell 2218. The galaxy has a spectroscopic redshift of similar to 4, and is currently the highest redshift SMG known. It is detected at all wavelengths from optical to submm, including the Spitzer IRAC bands. We discuss the properties of this galaxy, which is undergoing intense star formation at a rate similar to 600 M(circle dot)yr(-1). We also compare the properties to those of radio-preselected submm-bright galaxies. The z approximate to 4 result extends the redshift distribution of SMGs.

引用

页码：372 / +

页数：2

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