The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev-Zel'dovich Galaxy Clusters

被引：186

作者：

Hilton, M. ^{[1
,2
]}

Sifon, C. ^{[3
]}

Naess, S. ^{[4
]}

Madhavacheril, M. ^{[5
]}

Oguri, M. ^{[6
,7
,8
]}

Rozo, E. ^{[9
]}

Rykoff, E. ^{[10
,11
]}

Abbott, T. M. C. ^{[12
]}

Adhikari, S. ^{[10
,11
,13
]}

Aguena, M. ^{[14
,15
]}

Aiola, S. ^{[14
]}

Allam, S. ^{[16
]}

Amodeo, S. ^{[17
]}

Amon, A. ^{[10
]}

Annis, J. ^{[16
]}

Ansarinejad, B. ^{[18
]}

Aros-Bunster, C. ^{[3
]}

Austermann, J. E. ^{[19
]}

Avila, S. ^{[20
]}

Bacon, D. ^{[21
]}

Battaglia, N. ^{[17
]}

Beall, J. A. ^{[19
]}

Becker, D. T. ^{[19
]}

Bernstein, G. M. ^{[22
]}

Bertin, E. ^{[23
,24
]}

Bhandarkar, T. ^{[22
]}

Bhargava, S. ^{[25
]}

Bond, J. R. ^{[26
]}

Brooks, D. ^{[27
]}

Burke, D. L. ^{[10
,11
]}

Calabrese, E. ^{[28
]}

Carrasco Kind, M. ^{[29
,30
]}

Carretero, J. ^{[31
]}

Choi, S. K. ^{[17
,32
]}

Choi, A. ^{[33
]}

Conselice, C. ^{[34
,35
]}

Costa, L. N. da ^{[15
,36
]}

Costanzi, M. ^{[37
,38
]}

Crichton, D. ^{[1
,2
]}

Crowley, K. T. ^{[39
]}

Dunner, R. ^{[40
,41
]}

Denison, E. V. ^{[19
]}

Devlin, M. J. ^{[22
]}

Dicker, S. R. ^{[22
]}

Diehl, H. T. ^{[16
]}

Dietrich, J. P. ^{[42
]}

Doel, P. ^{[27
]}

Duff, S. M. ^{[19
]}

Duivenvoorden, A. J. ^{[43
]}

Dunkley, J. ^{[43
,44
]}

机构：

[1] Univ KwaZulu Natal, Astrophys Res Ctr, Westville Campus, ZA-4041 Durban, South Africa

[2] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Westville Campus, ZA-4041 Durban, South Africa

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

[4] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA

[5] Perimeter Inst Theoret Phys, Ctr Universe, Waterloo, ON N2L 2Y5, Canada

[6] Univ Tokyo, Res Ctr Early Universe, Tokyo 1130033, Japan

[7] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan

[8] Univ Tokyo, WPI, Kavli Inst Phys & Math Universe Kavli IPMU, Chiba 2778582, Japan

[9] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA

[10] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[11] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[12] Cerro Tololo Interamer Observ, NSFs Natl Opt Infrared Astron Res Lab, Casilla 603, La Serena, Chile

[13] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[14] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, SP, Brazil

[15] Lab Interinst E Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[16] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[17] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

[18] Univ Durham, Dept Phys, South Rd, Durham DH1 3LE, England

[19] NIST, Quantum Sensors Grp, 325 Broadway, Boulder, CO 80305 USA

[20] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[21] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[22] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[23] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[24] UPMC Univ Paris 06, Sorbonne Univ, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[25] Univ Sussex, Dept Phys & Astron, Pevensey Bldg, Brighton BN1 9QH, E Sussex, England

[26] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada

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

[28] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[29] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA

[30] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[31] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[32] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA

[33] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[34] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England

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

[36] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[37] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy

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

[39] Univ Calif Berkeley, Dept Phys, 366 LeConte Hall, Berkeley, CA 94720 USA

[40] Pontificia Univ Catolica Chile, Inst Astrofis, Fac Fis, Av Vicuna Mackenna 4860, Santiago 7820436, Chile

[41] Pontificia Univ Catolica Chile, Ctr Astroingn, Fac Fis, Av Vicuna Mackenna 4860, Santiago 7820436, Chile

[42] Ludwig Maximilians Univ Munchen, Fac Phys, Scheinerstr 1, D-81679 Munich, Germany

[43] Princeton Univ, Joseph Henry Labs Phys, Jadwin Hall, Princeton, NJ 08544 USA

[44] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA

[45] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[46] Lawrence Berkeley Natl Lab, One Cyclotron Rd, Berkeley, CA 94720 USA

[47] Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA

[48] Univ Oslo, Inst Theoret Astrophys, POB 1029 Blindern, NO-0315 Oslo, Norway

[49] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[50] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2021年 / 253卷 / 01期

基金：

新加坡国家研究基金会; 欧洲研究理事会; 欧盟地平线“2020”; 美国国家航空航天局; 加拿大创新基金会; 美国国家科学基金会; 日本科学技术振兴机构; 日本学术振兴会;

关键词：

Galaxy clusters; Cosmology; Large-scale structure of the universe; LENSING MASS CALIBRATION; GRAVITATIONALLY LENSED OBJECTS; 720 SQUARE DEGREES; ALL-SKY SURVEY; SIMILAR-TO; DARK ENERGY; DISTANT CLUSTERS; PHOTOMETRIC REDSHIFTS; VELOCITY DISPERSIONS; PHYSICAL-PROPERTIES;

D O I：

10.3847/1538-4365/abd023

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio >4 in 13,211 deg(2) of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multifrequency matched filter to 98 and 150 GHz maps constructed from ACT observations obtained from 2008 to 2018 and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z < 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ signal versus mass-scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M-500c > 3.8 x 10(14) M, evaluated at z = 0.5, for clusters detected at signal-to-noise ratio >5 in maps filtered at an angular scale of 24. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ signal mass-scaling relation, such as the Dark Energy Survey (4566 deg(2)), the Hyper Suprime-Cam Subaru Strategic Program (469 deg(2)), and the Kilo Degree Survey (825 deg(2)). We highlight some noteworthy objects in the sample, including potentially projected systems, clusters with strong lensing features, clusters with active central galaxies or star formation, and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10 Gyr.

引用

页数：25

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