The discovery of primeval large-scale structures with forming clusters at redshift 6

被引:196
作者
Ouchi, M
Shimasaku, K
Akiyama, M
Sekiguchi, K
Furusawa, H
Okamura, S
Kashikawa, N
Iye, M
Kodama, T
Saito, T
Sasaki, T
Simpson, C
Takata, T
Yamada, T
Yamanoi, H
Yoshida, M
Yoshida, M
机构
[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[2] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[3] Natl Astron Observ, Subaru Telescope, Hilo, HI 96720 USA
[4] Natl Astron Observ, Tokyo 1818588, Japan
[5] Univ Durham, Dept Phys, Durham DH1 3LE, England
[6] Japan Womens Univ, Fac Sci, Dept Math & Phys Sci, Tokyo 1128681, Japan
[7] Natl Astron Observ, Okayama Astrophys Observ, Okayama 7190232, Japan
关键词
galaxies : clusters : general; galaxies : formation; large-scale structure of universe;
D O I
10.1086/428499
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of primeval large- scale structures ( LSSs) including two protoclusters in a forming phase at. We carried out extensive deep narrowband imaging in the 1 deg(2) sky of the Subaru/ XMM- Newton Deep at z = 5.7 Field and obtained a cosmic map of 515 Lyalpha emitters ( LAEs) in a volume with a transverse dimension of and a depth of similar to 40 Mpc in comoving units. This cosmic map shows filamentary LSSs, including 180 Mpc x 180 Mpc clusters and surrounding 10 - 40 Mpc scale voids, similar to the present- day LSSs. Our spectroscopic follow- up observations identify overdense regions in which two dense clumps of LAEs with a sphere of 1 Mpc diameter in physical units are included. These clumps show about 130 times higher star formation rate density, mainly due to a large overdensity, similar to 80, of LAEs. These clumps would be clusters in a formation phase involving a burst of galaxy formation.
引用
收藏
页码:L1 / L4
页数:4
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