Discovery of hyperluminous infrared galaxies using Spitzer and SHARC-II

被引:0
作者
Borys, C [1 ]
Barnard, V [1 ]
Bian, C [1 ]
Blain, AW [1 ]
Brown, MJI [1 ]
Dey, A [1 ]
Dowell, CD [1 ]
Frayer, DT [1 ]
Higdon, J [1 ]
Higdon, S [1 ]
Jannuzi, B [1 ]
Le Fl'och, E [1 ]
Soifer, BT [1 ]
Phillips, TG [1 ]
机构
[1] CALTECH, Pasadena, CA 91125 USA
来源
PROCEEDINGS OF THE DUSTY AND MOLECULAR UNIVERSE: A PRELUDE TO HERSCHEL AND ALMA | 2005年 / 577卷
关键词
galaxy evolution; galaxy formation; starburst galaxies;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used observations taken as part of the Bootes Spitzer GTO program to pre-select high redshift luminous star-forming galaxy candidates. Subsequent ground-based sub-millimeter imaging using SHARC-II at the Caltech Submillimeter Observatory detected several objects, including one particularly exotic one: An extremely bright infrared galaxy with an apparent luminosity in excess of 10(13.5)L(circle dot). It has a spectral energy distribution similar to that of Arp 220, though appears to be at a much higher redshift. Although lensing is one possible explanation, this object has helped refine the selection method, and hints at a way to pre-select similar objects using Mid-IR silicate absorption features.
引用
收藏
页码:275 / 276
页数:2
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