The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1

被引：70

作者：

Gonzalez, Anthony H. ^{[1
]}

Gettings, Daniel P. ^{[1
]}

Brodwin, Mark ^{[2
]}

Eisenhardt, Peter R. M. ^{[3
]}

Stanford, S. A. ^{[4
,5
]}

Wylezalek, Dominika ^{[6
]}

Decker, Bandon ^{[2
]}

Marrone, Daniel P. ^{[7
]}

Moravec, Emily ^{[1
]}

O'Donnell, Christine ^{[7
]}

Stalder, Brian ^{[8
]}

Stern, Daniel ^{[3
]}

Abdulla, Zubair ^{[9
,10
]}

Brown, Gillen ^{[2
,11
]}

Carlstrom, John ^{[9
,10
]}

Chambers, Kenneth C. ^{[12
]}

Hayden, Brian ^{[13
]}

Lin, Yen-ting ^{[14
]}

Magnier, Eugene ^{[12
]}

Masci, Frank J. ^{[15
]}

Mantz, Adam B. ^{[16
,17
]}

McDonald, Michael ^{[18
]}

Mo, Wenli ^{[1
]}

Perlmutter, Saul ^{[13
,19
]}

Wright, Edward L. ^{[20
]}

Zeimann, Gregory R. ^{[21
]}

机构：

[1] Univ Florida, Dept Astron, 211 Bryant Space Ctr, Gainesville, FL 32611 USA

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

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

[4] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA

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

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

[7] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA

[8] LSST, 950 North Cherry Ave, Tucson, AZ 85719 USA

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

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

[11] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[12] Univ Hawaii Manoa, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[13] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd,MS 50B-4206, Berkeley, CA 94720 USA

[14] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan

[15] Infrared Proc & Anal Ctr, Caltech 100-22, Pasadena, CA 91125 USA

[16] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 382 Via Pueblo Mall, Stanford, CA 94305 USA

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

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

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

[20] UCLA Astron, POB 951547, Los Angeles, CA 90095 USA

[21] Univ Texas Austin, Hobby Eberly Telescope, Austin, TX 78712 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2019年 / 240卷 / 02期

基金：

英国科学技术设施理事会; 美国国家航空航天局; 美国国家科学基金会;

关键词：

galaxies: clusters: general; galaxies: distances and redshifts; galaxies: evolution; surveys; SUPERCOSMOS SKY SURVEY; STELLAR POPULATION SYNTHESIS; INTERACTION CROSS-SECTION; DARK-MATTER; X-RAY; HIGH-REDSHIFT; XMMXCS J2215.9-1738; LUMINOSITY FUNCTION; DENSITY RELATION; EVOLUTION;

D O I：

10.3847/1538-4365/aafad2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the Massive and Distant Clusters of WISE Survey (MaDCoWS), a search for galaxy clusters at 0.7 less than or similar to z less than or similar to 1.5 based upon data from the Wide-field Infrared Survey Explorer (WISE) mission. MaDCoWS is the first cluster survey capable of discovering massive clusters at these redshifts over the full extragalactic sky. The search is divided into two regions-the region of the extragalactic sky covered by Pan-STARRS (delta > - 30 degrees) and the remainder of the southern extragalactic sky at delta < -30 degrees for which shallower optical data from the SuperCOSMOS Sky Survey is available. In this paper, we describe the search algorithm, characterize the sample, and present the first MaDCoWS data release-catalogs of the 2433 highest amplitude detections in the WISE-Pan-STARRS region and the 250 highest amplitude detections in the WISE-SuperCOSMOS region. A total of 1723 of the detections from the WISE-Pan-STARRS sample have also been observed with the Spitzer Space Telescope, providing photometric redshifts and richnesses, and an additional 64 detections within the WISE-SuperCOSMOS region also have photometric redshifts and richnesses. Spectroscopic redshifts for 38 MaDCoWS clusters with IRAC photometry demonstrate that the photometric redshifts have an uncertainty of sigma(z)/(1 + z) similar or equal to 0.036. Combining the richness measurements with Sunyaev-Zel'dovich observations of MaDCoWS clusters, we also present a preliminary mass-richness relation that can be used to infer the approximate mass distribution of the full sample. The estimated median mass for the WISE-Pan-STARRS catalog is M-500 = 1.6(-0.8)(+0.7) x 10(14) M-circle dot, with the Sunyaev-Zel'dovich data confirming that we detect clusters with masses up to M-500 similar to 5 x 10(14) M-circle dot (M-200 similar to 10(15) M-circle dot).

引用

页数：25

共 153 条

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共 153 条

[1] THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY [J].

Abazajian, Kevork N. ;

Adelman-McCarthy, Jennifer K. ;

Agueros, Marcel A. ;

Allam, Sahar S. ;

Prieto, Carlos Allende ;

An, Deokkeun ;

Anderson, Kurt S. J. ;

Anderson, Scott F. ;

Annis, James ;

Bahcall, Neta A. ;

Bailer-Jones, C. A. L. ;

Barentine, J. C. ;

Bassett, Bruce A. ;

Becker, Andrew C. ;

Beers, Timothy C. ;

Bell, Eric F. ;

Belokurov, Vasily ;

Berlind, Andreas A. ;

Berman, Eileen F. ;

Bernardi, Mariangela ;

Bickerton, Steven J. ;

Bizyaev, Dmitry ;

Blakeslee, John P. ;

Blanton, Michael R. ;

Bochanski, John J. ;

Boroski, William N. ;

Brewington, Howard J. ;

Brinchmann, Jarle ;

Brinkmann, J. ;

Brunner, Robert J. ;

Budavari, Tamas ;

Carey, Larry N. ;

Carliles, Samuel ;

Carr, Michael A. ;

Castander, Francisco J. ;

Cinabro, David ;

Connolly, A. J. ;

Csabai, Istvan ;

Cunha, Carlos E. ;

Czarapata, Paul C. ;

Davenport, James R. A. ;

de Haas, Ernst ;

Dilday, Ben ;

Doi, Mamoru ;

Eisenstein, Daniel J. ;

Evans, Michael L. ;

Evans, N. W. ;

Fan, Xiaohui ;

Friedman, Scott D. ;

Frieman, Joshua A. .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2009, 182 (02) :543-558

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Abbott, T. ;

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Aleksic, J. ;

Allam, S. ;

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Bechtol, K. ;

Benoit-Levy, A. ;

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Bertin, E. ;

Blazek, J. ;

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Bridle, S. ;

Brooks, D. ;

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Buckley-Geer, E. ;

Burke, D. L. ;

Caminha, G. B. ;

Capozzi, D. ;

Carlsen, J. ;

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Carollo, M. ;

Carrasco-Kind, M. ;

Carretero, J. ;

Castander, F. J. ;

Clerkin, L. ;

Collett, T. ;

Conselice, C. ;

Crocce, M. ;

Cunha, C. E. ;

D'Andrea, C. B. ;

da Costa, L. N. ;

Davis, T. M. ;

Desai, S. ;

Diehl, H. T. ;

Dietrich, J. P. ;

Dodelson, S. ;

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Drlica-Wagner, A. ;

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Evrard, A. E. ;

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Flaugher, B. ;

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Abbott, T. M. C. ;

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da Costa, L. N. ;

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Barreiro, R. B. ;

Barrena, R. ;

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Benoit-Levy, A. ;

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Bersanelli, M. ;

Bielewicz, P. ;

Bikmaev, I. ;

Boehringer, H. ;

Bonaldi, A. ;

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Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Bucher, M. ;

Burenin, R. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

Cardoso, J. -F. ;

Carvalho, P. ;

Catalano, A. ;

Challinor, A. ;

Chamballu, A. ;

Chary, R. -R. ;

Chiang, H. C. ;

Chon, G. ;

Christensen, P. R. ;

Clements, D. L. ;

Colombi, S. ;

Colombo, L. P. L. ;

Combet, C. ;

Comis, B. ;

Couchot, F. ;

Coulais, A. ;

Crill, B. P. ;

Curto, A. ;

Cuttaia, F. .

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[5] Planck 2015 results XIII. Cosmological parameters [J].

Ade, P. A. R. ;

Aghanim, N. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Baccigalupi, C. ;

Banday, A. J. ;

Barreiro, R. B. ;

Bartlett, J. G. ;

Bartolo, N. ;

Battaner, E. ;

Battye, R. ;

Benabed, K. ;

Benoit, A. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bielewicz, P. ;

Bock, J. J. ;

Bonaldi, A. ;

Bonavera, L. ;

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