GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10

被引：151

作者：

Harikane, Yuichi ^{[1
,2
]}

Ono, Yoshiaki ^{[1
]}

Ouchi, Masami ^{[1
,3
,4
,5
]}

Liu, Chengze ^{[6
,7
]}

Sawicki, Marcin ^{[8
,9
]}

Shibuya, Takatoshi ^{[10
]}

Behroozi, Peter S. ^{[11
,12
]}

He, Wanqiu ^{[3
]}

Shimasaku, Kazuhiro ^{[13
,14
]}

Arnouts, Stephane ^{[15
]}

Coupon, Jean ^{[16
]}

Fujimoto, Seiji ^{[17
,18
]}

Gwyn, Stephen ^{[19
]}

Huang, Jiasheng ^{[20
,21
]}

Inoue, Akio K. ^{[22
,23
]}

Kashikawa, Nobunari ^{[13
,14
]}

Komiyama, Yutaka ^{[3
,4
]}

Matsuoka, Yoshiki ^{[24
]}

Willott, Chris J. ^{[19
]}

机构：

[1] Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778582, Japan

[2] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[3] Natl Astron Observ, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[4] Grad Univ Adv Studies SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[5] Univ Tokyo, Kavli Inst Phys & Math Universe Kavli IPMU, WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba, Japan

[6] Shanghai Jiao Tong Univ, Dept Astron, Sch Phys & Astron, Shanghai 200240, Peoples R China

[7] Shanghai Jiao Tong Univ, Shanghai Key Lab Particle Phys & Cosmol, Shanghai 200240, Peoples R China

[8] St Marys Univ, Inst Computat Astrophys, 923 Robie St, Halifax, NS B3H 3C3, Canada

[9] St Marys Univ, Dept Astron & Phys, 923 Robie St, Halifax, NS B3H 3C3, Canada

[10] Kitami Inst Technol, 165 Koen Cho, Kitami, Hokkaido 0908507, Japan

[11] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA

[12] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[13] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[14] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[15] Aix Marseille Univ, Lab Astrophys Marseille, CNES, CNRS, Marseille, France

[16] Univ Geneva, Astron Dept, Chemin Ecogia 16, CH-1290 Versoix, Switzerland

[17] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[18] Univ Copenhagen, Niels Bohr Inst, DK-128 Copenhagen, Denmark

[19] NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada

[20] Natl Astron Observ China, CASSACA, Beijing, Peoples R China

[21] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[22] Waseda Univ, Fac Sci & Engn, Sch Adv Sci & Engn, Dept Phys,Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

[23] Waseda Univ, Fac Sci & Engn, Waseda Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

[24] Ehime Univ, Res Ctr Space & Cosm Evolut, Bunkyo Cho, Matsuyama, Ehime 7908577, Japan

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2022年 / 259卷 / 01期

基金：

日本学术振兴会; 日本科学技术振兴机构; 美国国家科学基金会; 欧盟地平线“2020”; 美国国家航空航天局; 新加坡国家研究基金会;

关键词：

HIGH-Z EXPLORATION; LY-ALPHA EMITTERS; LYMAN-BREAK GALAXIES; HALO OCCUPATION DISTRIBUTION; DEEP SURVEY SXDS; FORMING GALAXIES; BRIGHT END; FAINT-END; SPECTROSCOPIC SURVEY; DATA RELEASE;

D O I：

10.3847/1538-4365/ac3dfc

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present new measurements of rest-UV luminosity functions and angular correlation functions from 4,100,221 galaxies at z similar to 2-7 identified in the Subaru/Hyper Suprime-Cam survey and CFHT Large Area U-band Survey. The obtained luminosity functions at z similar to 4-7 cover a very wide UV luminosity range of similar to 0.002-2000L(UV)(*) combined with previous studies, confirming that the dropout luminosity function is a superposition of the active galactic nucleus (AGN) luminosity function dominant at M-UV less than or similar to -24 mag and the galaxy luminosity function dominant at M-UV greater than or similar to -22 mag, consistent with galaxy fractions based on 1037 spectroscopically identified sources. Galaxy luminosity functions estimated from the spectroscopic galaxy fractions show the bright-end excess beyond the Schechter function at greater than or similar to 2 sigma levels, possibly made by inefficient mass quenching, low dust obscuration, and/or hidden AGN activity. By analyzing the correlation functions at z similar to 2-6 with HOD models, we find a weak redshift evolution (within 0.3 dex) of the ratio of the star formation rate (SFR) to the dark matter accretion rate, SFR/<(M)over dot>(h) 10 with proportional to 10(-0.5(1+z)), which will be directly tested with the James Webb Space Telescope.

引用

页数：37

共 253 条

[121] BIAS AND VARIANCE OF ANGULAR-CORRELATION FUNCTIONS [J].

LANDY, SD ;

SZALAY, AS .

ASTROPHYSICAL JOURNAL, 1993, 412 (01) :64-71

[122] A Spectroscopic Search for AGN Activity in the Reionization Era [J].

Laporte, Nicolas ;

Nakajima, Kimihiko ;

Ellis, Richard S. ;

Zitrin, Adi ;

Stark, Daniel P. ;

Mainali, Ramesh ;

Roberts-Borsani, G. W. .

ASTROPHYSICAL JOURNAL, 2017, 851 (01)

[123] The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z ∼ 6.7 selected with 17.5 ≤ iAB ≤ 24.75 [J].

Le Fevre, O. ;

Cassata, P. ;

Cucciati, O. ;

Garilli, B. ;

Ilbert, O. ;

Le Brun, V. ;

Maccagni, D. ;

Moreau, C. ;

Scodeggio, M. ;

Tresse, L. ;

Zamorani, G. ;

Adami, C. ;

Arnouts, S. ;

Bardelli, S. ;

Bolzonella, M. ;

Bondi, M. ;

Bongiorno, A. ;

Bottini, D. ;

Cappi, A. ;

Charlot, S. ;

Ciliegi, P. ;

Contini, T. ;

de la Torre, S. ;

Foucaud, S. ;

Franzetti, P. ;

Gavignaud, I. ;

Guzzo, L. ;

Iovino, A. ;

Lemaux, B. ;

Lopez-Sanjuan, C. ;

McCracken, H. J. ;

Marano, B. ;

Marinoni, C. ;

Mazure, A. ;

Mellier, Y. ;

Merighi, R. ;

Merluzzi, P. ;

Paltani, S. ;

Pello, R. ;

Pollo, A. ;

Pozzetti, L. ;

Scaramella, R. ;

Tasca, L. ;

Vergani, D. ;

Vettolani, G. ;

Zanichelli, A. ;

Zucca, E. .

ASTRONOMY & ASTROPHYSICS, 2013, 559

[124] Weak gravitational lensing with COSMOS:: Galaxy selection and shape measurements [J].

Leauthaud, Alexie ;

Massey, Richard ;

Kneib, Jean-Paul ;

Rhodes, Jason ;

Johnston, David E. ;

Capak, Peter ;

Heymans, Catherine ;

Ellis, Richard S. ;

Koekemoer, Anton M. ;

Le Fevre, Oliver ;

Mellier, Yannick ;

Refregier, Alexandre ;

Robin, Annie C. ;

Scoville, Nick ;

Tasca, Lidia ;

Taylor, James E. ;

Van Waerbeke, Ludovic .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2007, 172 (01) :219-238

[125] NEW CONSTRAINTS ON THE EVOLUTION OF THE STELLAR-TO-DARK MATTER CONNECTION: A COMBINED ANALYSIS OF GALAXY-GALAXY LENSING, CLUSTERING, AND STELLAR MASS FUNCTIONS FROM z=0.2 to z=1 [J].

Leauthaud, Alexie ;

Tinker, Jeremy ;

Bundy, Kevin ;

Behroozi, Peter S. ;

Massey, Richard ;

Rhodes, Jason ;

George, Matthew R. ;

Kneib, Jean-Paul ;

Benson, Andrew ;

Wechsler, Risa H. ;

Busha, Michael T. ;

Capak, Peter ;

Cortes, Marina ;

Ilbert, Olivier ;

Koekemoer, Anton M. ;

Le Fevre, Oliver ;

Lilly, Simon ;

McCracken, Henry J. ;

Salvato, Mara ;

Schrabback, Tim ;

Scoville, Nick ;

Smith, Tristan ;

Taylor, James E. .

ASTROPHYSICAL JOURNAL, 2012, 744 (02)

[126] The large-scale and small-scale clustering of Lyman break galaxies at 3.5 ≤ z ≤ 5.5 from the GOODS survey [J].

Lee, KS ;

Giavalisco, M ;

Gnedin, OY ;

Somerville, RS ;

Ferguson, HC ;

Dickinson, M ;

Ouchi, M .

ASTROPHYSICAL JOURNAL, 2006, 642 (01) :63-80

[127] The Anglo-Australian Observatory 2dF facility [J].

Lewis, IJ ;

Cannon, RD ;

Taylor, K ;

Glazebrook, K ;

Bailey, JA ;

Baldry, IK ;

Barton, JR ;

Bridges, TJ ;

Dalton, GB ;

Farrell, TJ ;

Gray, PM ;

Lankshear, A ;

McCowage, C ;

Parry, IR ;

Sharples, RM ;

Shortridge, K ;

Smith, GA ;

Stevenson, J ;

Straede, JO ;

Waller, LG ;

Whittard, JD ;

Wilcox, JK ;

Willis, KC .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 333 (02) :279-298

[128] OzDES multi-object fibre spectroscopy for the Dark Energy Survey: results and second data release [J].

Lidman, C. ;

Tucker, B. E. ;

Davis, T. M. ;

Uddin, S. A. ;

Asorey, J. ;

Bolejko, K. ;

Brout, D. ;

Calcino, J. ;

Carollo, D. ;

Carr, A. ;

Childress, M. ;

Hoormann, J. K. ;

Foley, R. J. ;

Galbany, L. ;

Glazebrook, K. ;

Hinton, S. R. ;

Kessler, R. ;

Kim, A. G. ;

King, A. ;

Kremin, A. ;

Kuehn, K. ;

Lagattuta, D. ;

Lewis, G. F. ;

Macaulay, E. ;

Malik, U. ;

March, M. ;

Martini, P. ;

Moller, A. ;

Mudd, D. ;

Nichol, R. C. ;

Panther, F. ;

Parkinson, D. ;

Pursiainen, M. ;

Sako, M. ;

Swann, E. ;

Scalzo, R. ;

Scolnic, D. ;

Sharp, R. ;

Smith, M. ;

Sommer, N. E. ;

Sullivan, M. ;

Webb, S. ;

Wiseman, P. ;

Yu, Z. ;

Yuan, F. ;

Zhang, B. ;

Abbott, T. M. C. ;

Aguena, M. ;

Allam, S. ;

Annis, J. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 496 (01) :19-35

[129]

Lilly SJ, 1996, ASTROPHYS J, V460, pL1, DOI 10.1086/309975

[130] Deriving the nonlinear cosmological power spectrum and bispectrum from analytic dark matter halo profiles and mass functions [J].

Ma, CP ;

Fry, JN .

ASTROPHYSICAL JOURNAL, 2000, 543 (02) :503-513

← 8 9 10 11 12 13 14 15 16 17 →

GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z &gt; 10

GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10