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SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z similar to 6-7: Strong Associations of Dusty Star-forming Galaxies

文献类型:期刊论文

作者Harikane, Yuichi28,29,30; Ouchi, Masami27,30; Ono, Yoshiaki30; Fujimoto, Seiji26,30; Donevski, Darko24,25; Shibuya, Takatoshi23; Faisst, Andreas L.22; Goto, Tomotsugu21; Hatsukade, Bunyo20; Kashikawa, Nobunari26
刊名ASTROPHYSICAL JOURNAL
出版日期2019-10-01
卷号883期号:2页码:16
ISSN号0004-637X
关键词galaxies: evolution galaxies: formation galaxies: high-redshift
DOI10.3847/1538-4357/ab2cd5
通讯作者Harikane, Yuichi(hari@icrr.u-tokyo.ac.jp)
英文摘要We have obtained three-dimensional maps of the universe in similar to 200 x 200 x 80 comoving Mpc(3) (cMpc(3)) volumes each at z = 5.7 and 6.6 based on a spectroscopic sample of 179 galaxies that achieves greater than or similar to 80% completeness down to the Ly alpha luminosity of log(L-Ly alpha/[erg s(-1)]) = 43.0, based on our Keck and Gemini observations and the literature. The maps reveal filamentary large-scale structures and two remarkable overdensities made out of at least 44 and 12 galaxies at z = 5.692 (z57OD) and z = 6.585 (z66OD), respectively, making z66OD the most distant overdensity spectroscopically confirmed to date, with >10 spectroscopically confirmed galaxies. We compare spatial distributions of submillimeter galaxies at z similar or equal to 4-6 with our z = 5.7 galaxies forming the large-scale structures, and detect a 99.97% signal of cross-correlation, indicative of a clear coincidence of dusty star-forming galaxy and dust-unobscured galaxy formation at this early epoch. The galaxies in z57OD and z66OD are actively forming stars with star-formation rates (SFRs) greater than or similar to 5 times higher than the main sequence, and particularly the SFR density in z57OD is 10 times higher than the cosmic average at the redshift (a.k.a. the Madau-Lilly plot). Comparisons with numerical simulations suggest that z57OD and z66OD are protoclusters that are progenitors of the present-day clusters with halo masses of similar to 10(14) M-circle dot.
WOS关键词LY-ALPHA EMITTERS ; LYMAN-BREAK GALAXIES ; RADIO GALAXY ; HIGH-REDSHIFT ; PROTO-CLUSTER ; ENVIRONMENTAL DEPENDENCE ; EMITTING GALAXIES ; NEBULAR EMISSION ; DENSITY RELATION ; DEEP SURVEY
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000498390600001
源URL[http://libir.pmo.ac.cn/handle/332002/35220]  
专题中国科学院紫金山天文台
通讯作者Harikane, Yuichi
作者单位1.Niels Bohr Inst, Cosm Dawn Ctr Dawn, Juliane Mariesvej 30, DK-2100 Copenhagen, Denmark
2.Ehime Univ, Res Ctr Space & Cosm Evolut, Bunkyo Cho, Matsuyama, Ehime 7908577, Japan
3.Nagoya Univ, Grad Sch Sci, Div Particle & Astrophys Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
4.NAOJ, Subaru Telescope, 650 N Aohoku P1, Hilo, HI 96720 USA
5.Onomichi City Univ, Dept Econ Management & Informat Sci, Hisayamada 1600-2, Onomichi, Hiroshima 7228506, Japan
6.Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China
7.Shanghai Jiao Tong Univ, Sch Phys & Astron, Tsung Dao Lee Inst, 800 Dongchuan Rd, Shanghai 200240, Peoples R China
8.Seoul Natl Univ, Dept Phys & Astron, CEOU Astron Program, Seoul, South Korea
9.Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England
10.Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 3J5, Canada
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Harikane, Yuichi,Ouchi, Masami,Ono, Yoshiaki,et al. SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z similar to 6-7: Strong Associations of Dusty Star-forming Galaxies[J]. ASTROPHYSICAL JOURNAL,2019,883(2):16.
APA Harikane, Yuichi.,Ouchi, Masami.,Ono, Yoshiaki.,Fujimoto, Seiji.,Donevski, Darko.,...&Wang, Wei-Hao.(2019).SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z similar to 6-7: Strong Associations of Dusty Star-forming Galaxies.ASTROPHYSICAL JOURNAL,883(2),16.
MLA Harikane, Yuichi,et al."SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z similar to 6-7: Strong Associations of Dusty Star-forming Galaxies".ASTROPHYSICAL JOURNAL 883.2(2019):16.

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