WISE Discovery of Hyper Luminous Galaxies at z=2-4 and Their Implications for Galaxy and AGN Evolution

被引:0
作者
Tsai, Chao-Wei [1 ]
Eisenhardt, Peter [2 ]
Wu, Jingwen [2 ]
Bridge, Carrie [3 ]
Assef, Roberto [2 ]
Benford, Dominic [4 ]
Blain, Andrew [5 ]
Cutri, Roc [1 ]
Griffith, Roger L. [1 ]
Jarrett, Thomas [1 ]
Lonsdale, Carol [6 ]
Petty, Sara [7 ]
Sayers, Jack
Stanford, Adam [8 ]
Stern, Daniel [2 ]
Wright, Edward L. [7 ]
Yan, Lin [1 ]
机构
[1] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA
[3] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[4] NASA, Goddard Space Flight Ctr, \, Greenbelt, MD 20771 USA
[5] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[6] Natl Radio Astron Observ, Charlottesville, VA 22901 USA
[7] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90024 USA
[8] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
来源
GALAXY MERGERS IN AN EVOLVING UNIVERSE | 2013年 / 477卷
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
On behalf of the WISE Science team, we present the discovery of a class of distant dust-enshrouded galaxies with extremely high luminosity. These galaxies are selected to have extreme red colors in the mid-IR using NASA's Wide-field Infrared Survey Explorer (WISE). They are faint in the optical and near-IR, predominantly at z=2-4, and with IR luminosity > 10(13)L(circle dot), making them Hyper-Luminous Infrared Galaxies (HyLIRGs). SEDs incorporating the WISE, Spitzer, and Herschel PACS and SPIRE photometry indicate hot dust dominates the bolometric luminosity, presumably powered by AGN. Preliminary multi-wavelength follow-up suggests that they are different from normal populations in the local M-sigma relation. Their low source density implies that these objects are either intrinsically rare, or a short-lived phase in a more numerous population. If the latter is the case, these hot, dust-enshrouded galaxies may be an early stage in the interplay between AGN and galaxies.
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页码:247 / +
页数:2
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