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arXiv · 1307.2903

SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation

M. B. Bayliss·M. L. N. Ashby·J. Ruel·M. Brodwin·K. A. Aird·M. W. Bautz·B. A. Benson·L. E. Bleem·S. Bocquet·J. E. Carlstrom·C. L. Chang·H. M. Cho·A. Clocchiatti·T. M. Crawford·A. T. Crites·S. Desai·M. A. Dobbs·J. P. Dudley·R. J. Foley·W. R. Forman·E. M. George·D. Gettings·M. D. Gladders·A. H. Gonzalez·T. de Haan·N. W. Halverson·F. W. High·G. P. Holder·W. L. Holzapfel·S. Hoover·J. D. Hrubes·C. Jones·M. Joy·R. Keisler·L. Knox·A. T. Lee·E. M. Leitch·J. Liu·M. Lueker·D. Luong-Van·A. Mantz·D. P. Marrone·K. Mawatari·M. McDonald·J. J. McMahon·J. Mehl·S. S. Meyer·E. D. Miller·L. Mocanu·J. J. Mohr·T. E. Montroy·S. S. Murray·S. Padin·T. Plagge·C. Pryke·C. L. Reichardt·A. Rest·J. E. Ruhl·B. R. Saliwanchik·A. Saro·J. T. Sayre·K. K. Schaffer·E. Shirokoff·J. Song·B. Stalder·R. Suhada·H. G. Spieler·S. A. Stanford·Z. Staniszewski·A. A. Stark·K. Story·C. W. Stubbs·A. van Engelen·K. Vanderlinde·J. D. Vieira·A. Vikhlinin·R. Williamson·O. Zahn·A. Zenteno
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Abstract

SPT-CLJ2040-4451 -- spectroscopically confirmed at z = 1.478 -- is the highest redshift galaxy cluster yet discovered via the Sunyaev-Zel'dovich effect. SPT-CLJ2040-4451 was a candidate galaxy cluster identified in the first 720 deg^2 of the South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey, and confirmed in follow-up imaging and spectroscopy. From multi-object spectroscopy with Magellan-I/Baade+IMACS we measure spectroscopic redshifts for 15 cluster member galaxies, all of which have strong [O II] 3727 emission. SPT-CLJ2040-4451 has an SZ-measured mass of M_500,SZ = 3.2 +/- 0.8 X 10^14 M_Sun/h_70, corresponding to M_200,SZ = 5.8 +/- 1.4 X 10^14 M_Sun/h_70. The velocity dispersion measured entirely from blue star forming members is sigma_v = 1500 +/- 520 km/s. The prevalence of star forming cluster members (galaxies with > 1.5 M_Sun/yr) implies that this massive, high-redshift cluster is experiencing a phase of active star formation, and supports recent results showing a marked increase in star formation occurring in galaxy clusters at z >1.4. We also compute the probability of finding a cluster as rare as this in the SPT-SZ survey to be >99%, indicating that its discovery is not in tension with the concordance Lambda-CDM cosmological model.

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M. B. Bayliss, M. L. N. Ashby, J. Ruel, M. Brodwin, K. A. Aird, M. W. Bautz, B. A. Benson, L. E. Bleem, S. Bocquet, J. E. Carlstrom, C. L. Chang, H. M. Cho, A. Clocchiatti, T. M. Crawford, A. T. Crites, S. Desai, M. A. Dobbs, J. P. Dudley, R. J. Foley, W. R. Forman, E. M. George, D. Gettings, M. D. Gladders, A. H. Gonzalez, T. de Haan, N. W. Halverson, F. W. High, G. P. Holder, W. L. Holzapfel, S. Hoover, J. D. Hrubes, C. Jones, M. Joy, R. Keisler, L. Knox, A. T. Lee, E. M. Leitch, J. Liu, M. Lueker, D. Luong-Van, A. Mantz, D. P. Marrone, K. Mawatari, M. McDonald, J. J. McMahon, J. Mehl, S. S. Meyer, E. D. Miller, L. Mocanu, J. J. Mohr, T. E. Montroy, S. S. Murray, S. Padin, T. Plagge, C. Pryke, C. L. Reichardt, A. Rest, J. E. Ruhl, B. R. Saliwanchik, A. Saro, J. T. Sayre, K. K. Schaffer, E. Shirokoff, J. Song, B. Stalder, R. Suhada, H. G. Spieler, S. A. Stanford, Z. Staniszewski, A. A. Stark, K. Story, C. W. Stubbs, A. van Engelen, K. Vanderlinde, J. D. Vieira, A. Vikhlinin, R. Williamson, O. Zahn, A. Zenteno. 2013-07-10. SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation. https://doi.org/10.1088/0004-637x/794/1/12

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