THE ERA OF STAR FORMATION IN GALAXY CLUSTERS by Brodwin, M., Stanford, S. A., Gonzalez, Anthony H., Zeimann, G. R., Snyder, G. F., Mancone, C. L., Pope, A., Eisenhardt, P. R., Stern, D., Alberts, S., Ashby, M. L. N., Brown, M. J. I., Chary, R.-R., Dey, A., Galametz, A., Gettings, D. P., Jannuzi, Buell T., Moustakas, J., Moustakas, L. A., Miller, Eric D

“…We analyze the star formation properties of 16 infrared-selected, spectroscopically confirmed galaxy clusters at 1 < z < 1.5 from the Spitzer/IRAC Shallow Cluster Survey (ISCS). …”
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COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY by Haan, T. de, Benson, B. A., Bleem, L. E., Allen, S. W., Applegate, D. E., Ashby, M. L. N., Bayliss, M., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H-M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., Dietrich, J. P., Dobbs, M. A., Doucouliagos, A. N., Foley, R. J., Forman, W. R., Garmire, G. P., George, E. M., Gladders, M. D., Gonzalez, A. H., Gupta, N., Halverson, N. W., Hlavacek-Larrondo, J., Hoekstra, H., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Huang, N., Jones, C., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Linden, von der A., Luong-Van, D., Mantz, A., Marrone, D. P., McMahon, J. J., Meyer, S. S., Mocanu, L. M., Mohr, J. J., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Shirokoff, E., Song, J., Spieler, H. G., Stalder, B., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K. T., Stubbs, C. W., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zenteno, A., McDonald, Michael A., Bautz, Marshall W.

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The Remarkable Similarity of Massive Galaxy Clusters from z ~ 0 to z ~ 1.9 by Allen, S. W., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gaspari, M., Gladders, M. D., Mantz, A. B., Murray, S. S., McDonald, Michael A., Bayliss, Matthew B, Bulbul, Gul E

“…We present the results of a Chandra X-ray survey of the eight most massive galaxy clusters at z > 1.2 in the South Pole Telescope 2500 deg[superscript 2] survey. …”
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THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 < by Haan, T. de, Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chiu, I., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gupta, N., Mohr, J. J., Reichardt, C. L., Saro, A., Vieira, J. D., Stalder, B., Stark, A. A., McDonald, Michael A., Bulbul, Gul E, Miller, Eric D

“…We present the results of an X-ray spectral analysis of 153 galaxy clusters observed with the Chandra, XMM-Newton, and Suzaku space telescopes. …”
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Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to z = 1.3 by Capasso, R., Saro, A., Mohr, J.J., Biviano, A., Bocquet, S., Strazzullo, V., Grandis, S., Applegate, D.E., Bayliss, Matthew B, Benson, B.A., Bleem, L.E., Brodwin, M., Bulbul, Esra, Carlstrom, J.E., Chiu, I., Dietrich, J.P., Gupta, N., de Haan, T., Hlavacek-Larrondo, J., Klein, M., von der Linden, A., McDonald, Michael A., Rapetti, D., Reichardt, C.L., Sharon, K., Stalder, B., Stanford, S.A., Stark, A.A., Stern, C., Zenteno, A., Bulbul, Esra

“…We present a dynamical study based on ~3000 passive, non-emission-line cluster galaxies drawn from 110 galaxy clusters. The galaxy clusters were selected using the Sunyaev-Zel'dovich effect (SZE) in the 2500 deg2 South Pole Telescope (SPT)-SZ survey and cover the redshift range 0.2 < z < 1.3. …”
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SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY by Bayliss, M. B., Ruel, J., Stubbs, C. W., Allen, S. W., Applegate, D. E., Ashby, M. L. N., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Capasso, R., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H-M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Haan, T. de, Desai, S., Dietrich, J. P., Dobbs, M. A., Doucouliagos, A. N., Foley, R. J., Forman, W. R., Garmire, G. P., George, E. M., Gladders, M. D., Gonzalez, A. H., Gupta, N., Halverson, N. W., Hlavacek-Larrondo, J., Hoekstra, H., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Huang, N., Jones, C., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Linden, A. von der, Luong-Van, D., Mantz, A., Marrone, D. P., McMahon, J. J., Meyer, S. S., Mocanu, L. M., Mohr, J. J., Murray, S. S., Padin, S., Pryke, C., Rapetti, D., Reichardt, C. L., Rest, A., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Shirokoff, E., Song, J., Spieler, H. G., Stalder, B., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K. T., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zenteno, A., McDonald, Michael A., Bautz, Marshall W.

“…The targets of SPT-GMOS are galaxy clusters identified in the SPT-SZ survey, a millimeter-wave survey of 2500 deg2 of the southern sky using the South Pole Telescope (SPT). …”
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Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-square-degree Survey by Huang, N., Bleem, L.E., Stalder, B., Ade, P.A.R., Allen, S.W., Anderson, A.J., Austermann, J.E., Avva, J.S., Beall, J.A., Bender, A.N., Benson, B.A., Bianchini, F., Bocquet, S., Brodwin, M., Carlstrom, J.E., Chang, C.L., Chiang, H.C., Citron, R., Corbett Moran, C., Crawford, T.M., Crites, A.T., de Haan, T., Dobbs, M.A., Everett, W., Floyd, B., Gallicchio, J., George, E.M., Gilbert, A., Gladders, M.D., Guns, S., Gupta, N., Halverson, N.W., Harrington, N., Henning, J.W., Hilton, G.C., Holder, G.P., Holzapfel, W.L., Hrubes, J.D., Hubmayr, J., Irwin, K.D., Khullar, G., Knox, L., Lee, A.T., Li, D., Lowitz, A., McDonald, Michael A., McMahon, J.J., Meyer, S.S., Mocanu, L.M., Montgomery, J., Nadolski, A., Natoli, T., Nibarger, J.P., Noble, G., Novosad, V., Padin, S., Patil, S., Pryke, C., Reichardt, C.L., Ruhl, J.E., Saliwanchik, B.R., Saro, A., Sayre, J.T., Schaffer, K.K., Sharon, K., Sievers, C., Smecher, G., Stark, A.A., Story, K.T., Tucker, C., Vanderlinde, K., Veach, T., Vieira, J.D., Wang, G., Whitehorn, N., Wu, W.L.K., Yefremenko, V.

“…We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. …”
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THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 < Z < 1.5 by Haan, T. de, Miller, E. D., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chiu, I., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gupta, N., Mohr, J. J., Reichardt, C. L., Saro, A., Stalder, B., Stark, A. A., Vieira, J. D., McDonald, Michael A., Bulbul, Gul E

“…We present the results of an X-ray spectral analysis of 153 galaxy clusters observed with the Chandra, XMM-Newton, and Suzaku space telescopes. …”
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Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 deg 2 SPT-SZ Survey by Khullar, G., Bleem, L.E., Bayliss, Matthew B, Gladders, M.D., Benson, B.A., McDonald, Michael A., Allen, S.W., Applegate, D.E., Ashby, M.L.N., Bocquet, S., Brodwin, M., Bulbul, Esra, Canning, R.E.A., Capasso, R., Chiu, I., Crawford, T.M., de Haan, T., Dietrich, J.P., Gonzalez, A.H., Hlavacek-Larrondo, J., Hoekstra, H., Holzapfel, W.L., von der Linden, A., Mantz, A.B., Patil, S., Reichardt, C.L., Saro, A., Sharon, K., Stalder, B., Stanford, S.A., Stark, A.A., Strazzullo, V.

“…We present spectroscopic confirmation of five galaxy clusters at 1.25 < z < 1.5, discovered in the 2500 deg2 South Pole Telescope Sunyaev-Zel'dovich (SZ) survey. …”
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THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. III. SUNYAEV-ZEL'DOVICH MASSES OF GALAXY CLUSTERS AT z ~ 1 by Brodwin, M., Greer, C. H., Leitch, E. M., Stanford, S. A., Gonzalez, A. H., Gettings, D. P., Abdulla, Z., Carlstrom, J. E., Decker, B., Eisenhardt, P. R., Lin, H.-W., Mantz, Adam B., Marrone, Daniel P., Stalder, B., Stern, D., Wylezalek, D., McDonald, Michael A.

“…We present CARMA 30 GHz Sunyaev–Zel'dovich (SZ) observations of five high-redshift (z [> over ~] 1), infrared-selected galaxy clusters discovered as part of the all-sky Massive and Distant Clusters of WISE Survey (MaDCoWS). …”
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X-RAY EMISSION FROM TWO INFRARED-SELECTED GALAXY CLUSTERS AT z > 1.4 IN THE IRAC SHALLOW CLUSTER SURVEY by Brodwin, M., Stern, D., Vikhlinin, A., Stanford, S. A., Gonzalez, Anthony H., Eisenhardt, P. R., Ashby, M. L. N., Bautz, Marshall W., Dey, A., Forman, W. R., Gettings, D. P., Hickox, R. C., Jannuzi, Buell T., Jones, C., Mancone, C. L., Moustakas, L. A., Ruel, J., Snyder, G., Zeimann, G., Miller, Eric D

“…We report the X-ray detection of two z > 1.4 infrared-selected galaxy clusters from the IRAC Shallow Cluster Survey (ISCS). …”
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Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters by Dietrich, J.P., Bocquet, S., Schrabback, T., Applegate, D., Hoekstra, H., Grandis, S., Mohr, J.J., Allen, S.W., Bayliss, Matthew B, Benson, B.A., Bleem, L.E., Brodwin, M., Bulbul, Esra, Capasso, R., Chiu, I., Crawford, T.M., Gonzalez, A.H., de Haan, T., Klein, M., von der Linden, A., Mantz, A.B., Marrone, D.P., McDonald, Michael A., Raghunathan, S., Rapetti, D., Reichardt, C.L., Saro, A., Stalder, B., Stark, A., Stern, C., Stubbs, C.

“…We present new ground-based weak lensing observations of 19 South Pole Telescope (SPT) selected clusters at redshifts 0.29 = z = 0.61 and combine them with previously reported space-based observations of 13 galaxy clusters at redshifts 0.576 = z = 1.132 to constrain the cluster mass scaling relations with the Sunyaev-Zel'dovich effect (SZE), the cluster gas mass Mgas and YX, the product of Mgas and X-ray temperature. …”
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SPT-CL J0546-5345: A MASSIVE z >1 GALAXY CLUSTER SELECTED VIA THE SUNYAEV-ZEL’DOVICH EFFECT WITH THE SOUTH POLE TELESCOPE by Andersson, Karl, Bautz, Marshall W., Brodwin, M., Ruel, J., Ade, P. A. R., Aird, K. A., Ashby, M. L. N., Bazin, G., Benson, Bradford A., Bleem, L. E.

“…The spectroscopic confirmation of SPT-CL J0546-5345, discovered in the wide-angle, mass-selected SPT cluster survey, marks the onset of the high-redshift SZE-selected galaxy cluster era.…”
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STAR-FORMING BRIGHTEST CLUSTER GALAXIES AT 0.25 < z < 1.25: A TRANSITIONING FUEL SUPPLY by Stalder, B., Bayliss, M., Allen, S. W., Applegate, D. E., Ashby, M. L. N., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chiu, I., Desai, S., Gonzalez, A. H., Hlavacek-Larrondo, J., Holzapfel, W. L., Marrone, D. P., Miller, E. D., Reichardt, C. L., Saliwanchik, B. R., Saro, A., Schrabback, T., Stanford, S. A., Stark, A. A., Vieira, J. D., Zenteno, A., McDonald, Michael A., Bautz, Marshall W.

“…We present a multiwavelength study of the 90 brightest cluster galaxies (BCGs) in a sample of galaxy clusters selected via the Sunyaev Zel'dovich effect by the South Pole Telescope, utilizing data from various ground- and space-based facilities. …”
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