THE MASSIVE DISTANT CLUSTERS OF WISE SURVEY: THE FIRST DISTANT GALAXY CLUSTER DISCOVERED BY WISE

被引：28

作者：

Gettings, Daniel P. ^{[1
]}

Gonzalez, Anthony H. ^{[1
]}

Stanford, S. Adam ^{[2
,3
]}

Eisenhardt, Peter R. M. ^{[4
]}

Brodwin, Mark ^{[5
]}

Mancone, Conor ^{[1
]}

Stern, Daniel ^{[4
]}

Zeimann, Gregory R. ^{[3
]}

Masci, Frank J. ^{[6
]}

Papovich, Casey ^{[7
,8
]}

Tanaka, Ichi ^{[9
]}

Wright, Edward L. ^{[10
]}

机构：

[1] Univ Florida, Dept Astron, Bryant Space Ctr 211, Gainesville, FL 32611 USA

[2] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA

[3] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[4] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[5] Univ Missouri, Dept Phys & Astron, Kansas City, MO 64110 USA

[6] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA

[7] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[8] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA

[9] Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA

[10] UCLA Astron, Los Angeles, CA 90095 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2012年 / 759卷 / 01期

基金：

美国国家航空航天局;

关键词：

galaxies: clusters: individual (MOO J2342.0+1301); galaxies: distances and redshifts; galaxies: evolution; STELLAR POPULATION SYNTHESIS; DIGITAL SKY SURVEY; DARK-MATTER; TELESCOPE; Z=1.75; RESOLUTION; EXISTENCE; UNIVERSE; CATALOG; MODELS;

D O I：

10.1088/2041-8205/759/1/L23

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present spectroscopic confirmation of a z = 0.99 galaxy cluster discovered using data from the Wide-field Infrared Survey Explorer (WISE). This is the first z similar to 1 cluster candidate from the Massive Distant Clusters of WISE Survey to be confirmed. It was selected as an overdensity of probable z greater than or similar to 1 sources using a combination of WISE and Sloan Digital Sky Survey DR8 photometric catalogs. Deeper follow-up imaging data from Subaru and WIYN reveal the cluster to be a rich system of galaxies, and multi-object spectroscopic observations from Keck confirm five cluster members at z = 0.99. The detection and confirmation of this cluster represents a first step toward constructing a uniformly selected sample of distant, high-mass galaxy clusters over the full extragalactic sky using WISE data.

引用

页数：6

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