NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < z < 4 in the COSMOS field

被引：4

作者：

Sillassen, Nikolaj B. ^{[1
,2
]}

Jin, Shuowen ^{[1
,2
]}

Magdis, Georgios E. ^{[1
,2
,3
]}

Daddi, Emanuele ^{[4
]}

Wang, Tao ^{[5
,6
]}

Lu, Shiying ^{[4
,5
,6
]}

Sun, Hanwen ^{[5
,6
]}

Arumugam, Vinod ^{[7
]}

Liu, Daizhong ^{[15
]}

Brinch, Malte ^{[1
,2
]}

D'Eugenio, Chiara ^{[9
,10
]}

Gobat, Raphael ^{[11
]}

Gomez-Guijarro, Carlos ^{[4
]}

Rich, Michael ^{[12
]}

Schinnerer, Eva ^{[8
]}

Strazzullo, Veronica ^{[13
,14
]}

Tan, Qinghua ^{[15
]}

Valentino, Francesco ^{[1
,16
]}

Wang, Yijun ^{[5
,6
]}

Xiao, Mengyuan ^{[17
]}

Zhou, Luwenjia ^{[5
,6
]}

Blanquez-Sese, David ^{[1
,2
]}

Cai, Zheng ^{[18
]}

Chen, Yanmei ^{[5
,6
]}

Ciesla, Laure ^{[4
]}

Dai, Yu ^{[19
]}

Delvecchio, Ivan ^{[20
,21
]}

Elbaz, David ^{[4
]}

Finoguenov, Alexis ^{[22
]}

Gao, Fangyou ^{[5
,6
]}

Gu, Qiusheng ^{[5
,6
]}

Hale, Catherine ^{[23
]}

Hao, Qiaoyang ^{[5
,6
]}

Huang, Jiasheng ^{[19
]}

Jarvis, Matt ^{[24
,25
]}

Kalita, Boris ^{[26
]}

Ke, Xu ^{[5
,6
]}

Le Bail, Aurelien ^{[4
]}

Magnelli, Benjamin ^{[4
]}

Shi, Yong ^{[5
,6
]}

Vaccari, Mattia ^{[27
]}

Whittam, Imogen ^{[24
,25
]}

Yang, Tiancheng ^{[5
,6
]}

Zhang, Zhiyu ^{[5
,6
]}

机构：

[1] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[2] Tech Univ Denmark, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark

[3] Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen, Denmark

[4] Univ Paris Saclay, Univ Paris Diderot, CNRS, AIM,CEA,Sorbonne Paris Cite, F-91191 Gif Sur Yvette, France

[5] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China

[6] Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Peoples R China

[7] IRAM, 300 rue piscine, F-38406 St Martin Dheres, France

[8] Max Planck Inst Extraterr Phys MPE, Giessenbachstr 1, D-85748 Garching, Germany

[9] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna 38205, Tenerife, Spain

[10] Univ Laguna, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain

[11] Pontificia Univ Catolica Valparaiso, Inst Fis, Casilla 4059, Valparaiso, Chile

[12] Univ Calif Los Angeles, Dept Phys & Astron, 430 Portola Plaza, Los Angeles, CA 90095 USA

[13] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste, Italy

[14] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34014 Trieste, Italy

[15] Chinese Acad Sci, Purple Mt Observ, 10 Yuanhua Rd, Nanjing 210023, Peoples R China

[16] European Southern Observ, Karl-Schwarzschild-Str 2, D-85748 Munich, Germany

[17] Univ Geneva, Dept Astron, Chemin Pegasi 51, CH-1290 Versoix, Switzerland

[18] Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China

[19] Chinese Acad Sci South Amer Ctr Astron CASSACA, Natl Astron Observ China NAOC, 20A Datun Rd, Beijing 100101, Peoples R China

[20] INAF Osservatorio Astron Brera, Via Brera 28, I-20121 Milan, Italy

[21] INAF Osservatorio Astron Brera, Via Bianchi 46, I-23807 Merate, Italy

[22] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, FI-00014 Helsinki, Finland

[23] Univ Edinburgh, Inst Astron, Sch Phys & Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Scotland

[24] Univ Oxford, Sub Dept Astrophys, Keble Rd, Oxford OX1 3RH, England

[25] Univ Western Cape, Dept Phys & Astron, Robert Sobukwe Rd, ZA-7535 Cape Town, South Africa

[26] Univ Tokyo, Kavli IPMU WPI, UTIAS, Kashiwa, Chiba 2778583, Japan

[27] Univ Western Cape, Interuniv Inst Data Intens Astron, Dept Phys & Astron, ZA-7535 Cape Town, South Africa

来源：

ASTRONOMY & ASTROPHYSICS | 2024年 / 690卷

基金：

中国国家自然科学基金; 新加坡国家研究基金会; 国家重点研发计划;

关键词：

galaxies: clusters: general; galaxies: evolution; galaxies: high-redshift; submillimeter: galaxies; EVOLVING INTERSTELLAR-MEDIUM; DEBLENDED DUST EMISSION; DARK ENERGY SURVEY; STELLAR MASS; SPECTROSCOPIC CONFIRMATION; CL J1449+0856; QUIESCENT GALAXIES; DENSITY PROFILE; MATTER HALOS; COLD STREAMS;

D O I：

10.1051/0004-6361/202450760

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at z>2 in six deep fields. We report spectroscopic confirmation of eight groups at 1.65 <= z <= 3.61 in COSMOS. Homogeneously selected as significant overdensities of red IRAC sources with red Herschel colors, four groups are confirmed by CO and [CI] with NOEMA 3mm observations, three are confirmed with ALMA, and one is confirmed by H alpha from Subaru/FMOS. We constructed the integrated FIR SEDs for the eight groups, obtaining total IR SFR =260-1300 M-circle dot similar to yr(-1). We adopted six methods to estimate the dark matter masses, including stellar mass to halo mass relations, overdensity with galaxy bias, and NFW profile fitting to radial stellar mass density. We found the radial stellar mass density are consistent with a NFW profile, supporting that they are collapsed structures hosted by a single dark matter halo. The best halo mass estimates are log(M-h/M-circle dot)=12.8-13.7 with uncertainty of 0.3 dex. From halo mass estimates, we derive baryonic accretion rate BAR=(1-8)x10(3) M-circle dot/yr for this sample. We find a quasi-linear correlation between the integrated SFR/BAR and the theoretical halo mass limit for cold streams, M-stream/M-h, with SFR/BAR=10(-0.46 +/- 0.22)(M-stream/M-h)(0.71 +/- 0.16) with a scatter of 0.40dex. Further, we compare halo masses and stellar masses with simulations, and find all structures are consistent with being progenitors of M-h(z=0) > 10(14) M-circle dot galaxy clusters, and the most massive central galaxies have stellar masses consistent with brightest cluster galaxies (BCGs) progenitors in the TNG300 simulation. The results strongly suggest these structures are forming massive galaxy clusters via baryonic and dark matter accretion.

引用

页数：35

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NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 &lt; z &lt; 4 in the COSMOS field

NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < z < 4 in the COSMOS field