Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-square-degree Survey

被引：60

作者：

Huang, N. ^{[1
]}

Bleem, L. E. ^{[2
,3
]}

Stalder, B. ^{[4
,5
]}

Ade, P. A. R. ^{[6
]}

Allen, S. W. ^{[7
,8
,9
]}

Anderson, A. J. ^{[10
]}

Austermann, J. E. ^{[11
]}

Avva, J. S. ^{[1
]}

Beall, J. A. ^{[11
]}

Bender, A. N. ^{[2
,3
]}

Benson, B. A. ^{[3
,10
,12
]}

Bianchini, F. ^{[13
]}

Bocquet, S. ^{[2
,3
,14
]}

Brodwin, M. ^{[15
]}

Carlstrom, J. E. ^{[2
,3
,12
,16
,17
]}

Chang, C. L. ^{[2
,3
,12
]}

Chiang, H. C. ^{[18
,19
]}

Citron, R. ^{[20
]}

Moran, C. Corbett ^{[20
,21
]}

Crawford, T. M. ^{[3
,12
]}

Crites, A. T. ^{[3
,12
,22
]}

de Haan, T. ^{[1
,23
]}

Dobbs, M. A. ^{[18
,24
]}

Everett, W. ^{[25
]}

Floyd, B. ^{[15
]}

Gallicchio, J. ^{[3
,26
]}

George, E. M. ^{[1
,27
]}

Gilbert, A. ^{[18
]}

Gladders, M. D. ^{[3
,12
]}

Guns, S. ^{[1
]}

Gupta, N. ^{[13
]}

Halverson, N. W. ^{[25
,28
]}

Harrington, N. ^{[1
]}

Henning, J. W. ^{[2
,3
]}

Hilton, G. C. ^{[11
]}

Holder, G. P. ^{[24
,29
,30
]}

Holzapfel, W. L. ^{[1
]}

Hrubes, J. D. ^{[20
]}

Hubmayr, J. ^{[11
]}

Irwin, K. D. ^{[8
,9
]}

Khullar, G. ^{[3
,12
]}

Knox, L. ^{[31
]}

Lee, A. T. ^{[1
,23
]}

Li, D. ^{[9
,11
]}

Lowitz, A. ^{[12
]}

McDonald, M. ^{[32
]}

McMahon, J. J. ^{[33
]}

Meyer, S. S. ^{[3
,12
,16
,17
]}

Mocanu, L. M. ^{[3
,12
,34
]}

Montgomery, J. ^{[18
]}

机构：

[1] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[2] Argonne Natl Lab, Div High Energy Phys, 9700 S Cass Ave, Argonne, IL 60439 USA

[3] Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[4] LSST, 950 N Cherry Ave, Tucson, AZ USA

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

[6] Cardiff Univ, Cardiff CF10 3XQ, Wales

[7] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA

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

[9] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA

[10] Fermilab Natl Accelerator Lab, MS209,POB 500, Batavia, IL 60510 USA

[11] NIST Quantum Devices Grp, 325 Broadway Mailcode 817-03, Boulder, CO 80305 USA

[12] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[13] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia

[14] Ludwig Maximilians Univ Munchen, Dept Phys, Scheinerstr 1, D-81679 Munich, Germany

[15] Univ Missouri, Dept Phys & Astron, 5110 Rockhill Rd, Kansas City, MO 64110 USA

[16] Univ Chicago, Dept Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[17] Univ Chicago, Enrico Fermi Inst, 5640 South Ellis Ave, Chicago, IL 60637 USA

[18] McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada

[19] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Durban, South Africa

[20] Univ Chicago, 5640 South Ellis Ave, Chicago, IL 60637 USA

[21] CALTECH, Walter Burke Inst Theoret Phys, TAPIR, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[22] CALTECH, MS 249-17,1216 E Calif Blvd, Pasadena, CA 91125 USA

[23] Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA

[24] CIFAR Program Cosmol & Grav, Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada

[25] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA

[26] Harvey Mudd Coll, 301 Platt Blvd, Claremont, CA 91711 USA

[27] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[28] Univ Colorado, Dept Phys, Boulder, CO 80309 USA

[29] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA

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

[31] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA 95616 USA

[32] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA

[33] Univ Michigan, Dept Phys, 450 Church St, Ann Arbor, MI 48109 USA

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

[35] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[36] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA

[37] Univ Minnesota, Sch Phys & Astron, 116 Chruch St SE, Minneapolis, MN 55455 USA

[38] Case Western Reserve Univ, Dept Phys, Ctr Educ & Res Cosmol & Astrophys, Cleveland, OH 44106 USA

[39] Yale Univ, Dept Phys, 217 Prospect St, New Haven, CT 06511 USA

[40] Univ Trieste, Dept Phys, Astron Unit, Via Tiepolo 11, I-34131 Trieste, Italy

[41] IFPU, Via Beirut 2, I-34014 Trieste, Italy

[42] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, I-34143 Trieste, Italy

[43] Sch Art Inst Chicago, Liberal Arts Dept, 112 S Michigan Ave, Chicago, IL 60603 USA

[44] Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA

[45] Three Speed Log Inc, Victoria, BC V85 3Z5, Canada

[46] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M55 3H4, Canada

[47] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[48] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

来源：

ASTRONOMICAL JOURNAL | 2020年 / 159卷 / 03期

基金：

美国国家航空航天局; 美国国家科学基金会; 澳大利亚研究理事会; 加拿大自然科学与工程研究理事会;

关键词：

MICROWAVE BACKGROUND ANISOTROPIES; DATA RELEASE; SKY; COSMOLOGY; CATALOG; TIME; MASS;

D O I：

10.3847/1538-3881/ab6a96

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. The catalog contains 89 candidates detected with a signal-to-noise ratio greater than 4.6. The candidates are selected using the Sunyaev Zel'dovich effect at 95 and 150 GHz. Using both space- and ground -based optical and infrared telescopes, we have confirmed 81 candidates as galaxy clusters. We use these follow-up images and archival images to estimate photometric redshifts for 66 galaxy clusters and spectroscopic observations to obtain redshifts for 13 systems. An additional two galaxy clusters are confirmed using the overdensity of near-infrared galaxies only and are presented without redshifts. We find that 15 candidates (18% of the total sample) are at redshift z > 1.0, with a maximum confirmed redshift of zma, = 1.38 0.10. We expect this catalog to contain every galaxy cluster with Msooc > 2.6 x 1014Mo h701 and z > 0.25 in the survey area. The mass threshold is approximately constant above z = 0.25, and the complete catalog has a median mass of approximately 714-500c = 2.7 x 1014Mo h7-01. Compared to previous SPT works, the increased depth of the millimeter-wave data (11.2 and 6.5 K-arcmin at 95 and 150 GHz, respectively) makes it possible to find more galaxy clusters at high redshift and lower mass.

引用

页数：16

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