The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters

被引：0

作者：

Edward, Adit H. ^{[1
,2
]}

Balogh, Michael L. ^{[1
,2
]}

Bahe, Yannick M. ^{[3
,4
]}

Cooper, M. C. ^{[5
]}

Hatch, Nina A. ^{[6
]}

Marchioni, Justin ^{[1
,2
]}

Muzzin, Adam ^{[4
,7
]}

Noble, Allison ^{[8
]}

Rudnick, Gregory H. ^{[9
]}

Vulcani, Benedetta ^{[10
]}

Wilson, Gillian ^{[11
]}

De Lucia, Gabriella ^{[12
]}

Demarco, Ricardo ^{[13
]}

Forrest, Ben ^{[14
]}

Hirschmann, Michaela ^{[15
]}

Castignani, Gianluca ^{[16
,17
]}

Cerulo, Pierluigi ^{[18
]}

Finn, Rose A. ^{[19
]}

Hewitt, Guillaume ^{[1
,2
]}

Jablonka, Pascale ^{[20
,21
]}

Kodama, Tadayuki ^{[22
]}

Maurogordato, Sophie ^{[23
]}

Nantais, Julie ^{[24
]}

Xie, Lizhi ^{[25
]}

机构：

[1] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada

[2] Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L3G1, Canada

[3] Ecole Polytech Fed Lausanne EPFL, Inst Phys, Astrophys Lab, Observatoire Sauverny, CH-1290 Versoix, Switzerland

[4] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands

[5] Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92697 USA

[6] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England

[7] York Univ, Dept Phys & Astron, 4700,St, Keele, ON MJ3 IP3, Canada

[8] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA

[9] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[10] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[11] Univ Calif Merced, Dept Phys, 5200 Lake Rd, Merced, CA 95343 USA

[12] INAF Astron Observ Trieste, Via G B Tiepolo 11, I-34143 Trieste, Italy

[13] Univ Concepcion, Fac Ciencias Fisicas & Matemat, Dept Astron, Concepcion, Chile

[14] Univ Calif Davis, Dept Phys & Astron, 1 Shields Ave, Davis, CA 95616 USA

[15] Ecole Polytechn Fed Lausanne, Inst Phys, Lab Galaxy Evolut & Spectral Modelling, Observatoire Sauverny, Chemin Pegasi 51, CH-1290 Versoix, Switzerland

[16] Alma Mater Studiorum Univ Bologna, Dipartimento Fis Astron Augusto Righi, Via Gobetti 93-2, I-40129 Bologna, Italy

[17] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Gobetti 93-3, I-40129 Bologna, Italy

[18] Univ Concepcion, Fac Ingn, Dept Ingn Informat & Ciencias Computaci, Casilla 160-C, Concepcion, Chile

[19] Siena Coll, Dept Phys & Astron, 515 Loudon Rd, Loudonville, NY 12211 USA

[20] Ecole Polytech Fed Lausanne EPFL, Lab Astrophys, CH-1290 Sauverny, Switzerland

[21] Univ PSL, CNRS, GEPI, Observ Paris, Pl Jules Janssen, F-92190 Meudon, France

[22] Tohoku Univ, Astron Inst, 6-3 Aramaki, Sendai, Miyagi 9808578, Japan

[23] Univ Cote dAzur, CNRS, Lab Lagrange, Bd Observ,Observ Cote Azur,CS 34229, F-06304 Nice 4, France

[24] Univ Andres Bello, Inst Astrofis, Dept Ciencias Fis, Fernandez Concha 700, Santiago 7591538, Metropolitana, Chile

[25] Tianjin Normal Univ, Tianjin Astrophys Ctr, Binshuixidao 393, Tianjin 300387, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2023年 / 527卷 / 03期

基金：

美国国家科学基金会; 加拿大自然科学与工程研究理事会;

关键词：

galaxies: clusters: general; galaxies: evolution; OPTICAL LUMINOSITY DENSITY; STAR-FORMATION RATES; RED SEQUENCE; SYSTEMATIC SEARCH; CLUSTER CORES; DARK-MATTER; BLACK-HOLES; HALO MASS; EVOLUTION; ORIGIN;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an analysis of the galaxy stellar mass function (SMF) of 14 known protoclusters between 2.0 < z < 2.5 in the COSMOS field, down to a mass limit of 10(9.5) M-circle dot. We use existing photometric redshifts with a statistical background subtraction, and consider star-forming and quiescent galaxies identified from (NUV - r) and (r - J) colours separately. Our fiducial sample includes galaxies within 1 Mpc of the cluster centres. The shape of the protocluster SMF of star-forming galaxies is indistinguishable from that of the general field at this redshift. Quiescent galaxies, however, show a flatter SMF than in the field, with an upturn at low mass, though this is only significant at similar to 2 sigma. There is no strong evidence for a dominant population of quiescent galaxies at any mass, with a fraction <15 per cent at 1sconfidence for galaxies with log M-*/M-circle dot < 10.5. We compare our results with a sample of galaxy groups at 1 < z < 1.5, and demonstrate that a significant amount of environmental quenching must take place between these epochs, increasing the relative abundance of high-mass (M-*> 10(10.5) M-circle dot) quiescent galaxies by a factor greater than or similar to 2. However, we find that at lower masses (M-*< 1010.5 M-circle dot), no additional environmental quenching is required.

引用

页码：8598 / 8617

页数：20

共 50 条

[1] The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
Edward A.H.
Balogh M.L.
Bahe Y.M.
Cooper M.C.
Hatch N.A.
Marchioni J.
Muzzin A.
Noble A.
Rudnick G.H.
Vulcani B.
Wilson G.
De Lucia G.
Demarco R.
Forrest B.
Hirschmann M.
Castignani G.
Cerulo P.
Finn R.A.
Hewitt G.
Jablonka P.
Kodama T.
Maurogordato S.
Nantais J.
Xie L.
Monthly Notices of the Royal Astronomical Society, 2024, 527 (03) : 8598 - 8617
[2] MOIRCS Deep Survey. X. Evolution of Quiescent Galaxies as a Function of Stellar Mass at 0.5 < z < 2.5
Kajisawa, Masaru
Ichikawa, Takashi
Yoshikawa, Tomohiro
Yamada, Toru
Onodera, Masato
Akiyama, Masayuki
Tanaka, Ichi
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2011, 63 : S403 - S414
[3] THE SCALING OF STELLAR MASS AND CENTRAL STELLAR VELOCITY DISPERSION FOR QUIESCENT GALAXIES AT z < 0.7
Zahid, H. Jabran
Geller, Margaret J.
Fabricant, Daniel G.
Hwang, Ho Seong
ASTROPHYSICAL JOURNAL, 2016, 832 (02):
[4] Stellar Mass Profiles of Quiescent Galaxies in Different Environments at z ∼ 0
Mosleh, Moein
Tavasoli, Saeed
Tacchella, Sandro
ASTROPHYSICAL JOURNAL, 2018, 861 (02):
[5] Protoclusters with evolved populations around radio galaxies at z ∼ 2.5
Kajisawa, Masaru
Kodama, Tadayuki
Tanaka, Ichi
Yamada, Toru
Bower, Richard
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 371 (02) : 577 - 582
[6] THE STELLAR MASS FUNDAMENTAL PLANE AND COMPACT QUIESCENT GALAXIES AT z < 0.6
Zahid, H. Jabran
Damjanov, Ivana
Geller, Margaret J.
Hwang, Ho Seong
Fabricant, Daniel G.
ASTROPHYSICAL JOURNAL, 2016, 821 (02):
[7] Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
Lapi, A.
Mancuso, C.
Bressan, A.
Danese, L.
ASTROPHYSICAL JOURNAL, 2017, 847 (01):
[8] STELLAR KINEMATICS OF z ∼ 2 GALAXIES AND THE INSIDE-OUT GROWTH OF QUIESCENT GALAXIES
van de Sande, Jesse
Kriek, Mariska
Franx, Marijn
van Dokkum, Pieter G.
Bezanson, Rachel
Bouwens, Rychard J.
Quadri, Ryan F.
Rix, Hans-Walter
Skelton, Rosalind E.
ASTROPHYSICAL JOURNAL, 2013, 771 (02):
[9] Stellar content of extremely red quiescent galaxies at z > 2
Lopez-Corredoira, M.
Vazdekis, A.
Gutierrez, C. M.
Castro-Rodriguez, N.
ASTRONOMY & ASTROPHYSICS, 2017, 600
[10] Distant z > 2 protoclusters and their galaxies
Miley, G
Overzier, R
Venemans, B
Zirm, A
Rottgering, H
Ford, H
PENETRATING BARS THROUGH MASKS OF COSMIC DUST: THE HUBBLE TUNING FORK STRIKES A NEW NOTE, 2004, 319 : 477 - 487

← 1 2 3 4 5 →