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1. COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

Author: de Haan, T, Benson, BA, Bleem, LE, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Bayliss, M, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, Dobbs, MA, Doucouliagos, AN, Foley, RJ, Forman, WR, Garmire, GP, George, EM, Gladders, MD, Gonzalez, AH, Gupta, N, Halverson, NW, Hlavacek-Larrondo, J, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, von der Linden, A, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Rapetti, D, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zenteno, A, de Haan, T, Benson, BA, Bleem, LE, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Bayliss, M, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, Dobbs, MA, Doucouliagos, AN, Foley, RJ, Forman, WR, Garmire, GP, George, EM, Gladders, MD, Gonzalez, AH, Gupta, N, Halverson, NW, Hlavacek-Larrondo, J, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, von der Linden, A, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Rapetti, D, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, and Zenteno, A
Published: 2016

2. SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY

Author: Bayliss, MB, Ruel, J, Stubbs, CW, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Capasso, R, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Doucouliagos, AN, Foley, RJ, Forman, WR, Garmire, GP, George, EM, Gladders, MD, Gonzalez, AH, Gupta, N, Halverson, NW, Hlavacek-Larrondo, J, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, von der Linden, A, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Rapetti, D, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zenteno, A, Bayliss, MB, Ruel, J, Stubbs, CW, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Capasso, R, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Doucouliagos, AN, Foley, RJ, Forman, WR, Garmire, GP, George, EM, Gladders, MD, Gonzalez, AH, Gupta, N, Halverson, NW, Hlavacek-Larrondo, J, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, von der Linden, A, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Rapetti, D, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, and Zenteno, A
Published: 2016

3. A MEASUREMENT OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND BY GALAXY CLUSTERS USING DATA FROM THE SOUTH POLE TELESCOPE

Author: Baxter, EJ, Keisler, R, Dodelson, S, Aird, KA, Allen, SW, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, de Haan, T, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, Hennig, C, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Jones, C, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Millea, M, Mocanu, LM, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Baxter, EJ, Keisler, R, Dodelson, S, Aird, KA, Allen, SW, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, H-M, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, de Haan, T, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, Hennig, C, Hoekstra, H, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Jones, C, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Millea, M, Mocanu, LM, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: Clusters of galaxies are expected to gravitationally lens the cosmic microwave background (CMB) and thereby generate a distinct signal in the CMB on arcminute scales. Measurements of this effect can be used to constrain the masses of galaxy clusters with CMB data alone. Here we present a measurement of lensing of the CMB by galaxy clusters using data from the South Pole Telescope (SPT). We develop a maximum likelihood approach to extract the CMB cluster lensing signal and validate the method on mock data. We quantify the effects on our analysis of several potential sources of systematic error and find that they generally act to reduce the best-fit cluster mass. It is estimated that this bias to lower cluster mass is roughly $0.85\sigma$ in units of the statistical error bar, although this estimate should be viewed as an upper limit. We apply our maximum likelihood technique to 513 clusters selected via their SZ signatures in SPT data, and rule out the null hypothesis of no lensing at $3.1\sigma$. The lensing-derived mass estimate for the full cluster sample is consistent with that inferred from the SZ flux: $M_{200,\mathrm{lens}} = 0.83_{-0.37}^{+0.38}\, M_{200,\mathrm{SZ}}$ (68% C.L., statistical error only).
Published: 2015

4. Analysis of Sunyaev-Zel'dovich effect mass-observable relations using South Pole Telescope observations of an X-ray selected sample of low-mass galaxy clusters and groups

Author: Liu, J, Mohr, J, Saro, A, Aird, KA, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Foley, RJ, Gangkofner, D, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, L, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, Suhada, R, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Liu, J, Mohr, J, Saro, A, Aird, KA, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Foley, RJ, Gangkofner, D, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, L, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, Suhada, R, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: (Abridged) We use 95, 150, and 220GHz observations from the SPT to examine the SZE signatures of a sample of 46 X-ray selected groups and clusters drawn from ~6 deg^2 of the XMM-BCS. These systems extend to redshift z=1.02, have characteristic masses ~3x lower than clusters detected directly in the SPT data and probe the SZE signal to the lowest X-ray luminosities (>10^42 erg s^-1) yet. We develop an analysis tool that combines the SZE information for the full ensemble of X-ray-selected clusters. Using X-ray luminosity as a mass proxy, we extract selection-bias corrected constraints on the SZE significance- and Y_500-mass relations. The SZE significance- mass relation is in good agreement with an extrapolation of the relation obtained from high mass clusters. However, the fit to the Y_500-mass relation at low masses, while in good agreement with the extrapolation from high mass SPT clusters, is in tension at 2.8 sigma with the constraints from the Planck sample. We examine the tension with the Planck relation, discussing sample differences and biases that could contribute. We also present an analysis of the radio galaxy point source population in this ensemble of X-ray selected systems. We find 18 of our systems have 843 MHz SUMSS sources within 2 arcmin of the X-ray centre, and three of these are also detected at significance >4 by SPT. Of these three, two are associated with the group brightest cluster galaxies, and the third is likely an unassociated quasar candidate. We examine the impact of these point sources on our SZE scaling relation analyses and find no evidence of biases. We also examine the impact of dusty galaxies using constraints from the 220 GHz data. The stacked sample provides 2.8$\sigma$ significant evidence of dusty galaxy flux, which would correspond to an average underestimate of the SPT Y_500 signal that is (17+-9) per cent in this sample of low mass systems.
Published: 2015

5. MEASUREMENT OF GALAXY CLUSTER INTEGRATED COMPTONIZATION AND MASS SCALING RELATIONS WITH THE SOUTH POLE TELESCOPE

Author: Saliwanchik, BR, Montroy, TE, Aird, KA, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Nurgaliev, D, Padin, S, Patej, A, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Saliwanchik, BR, Montroy, TE, Aird, KA, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Nurgaliev, D, Padin, S, Patej, A, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: We describe a method for measuring the integrated Comptonization (YSZ) of clusters of galaxies from measurements of the Sunyaev-Zel'dovich (SZ) effect in multiple frequency bands and use this method to characterize a sample of galaxy clusters detected in South Pole Telescope (SPT) data. We test this method on simulated cluster observations and verify that it can accurately recover cluster parameters with negligible bias. In realistic simulations of an SPT-like survey, with realizations of cosmic microwave background anisotropy, point sources, and atmosphere and instrumental noise at typical SPT-SZ survey levels, we find that YSZ is most accurately determined in an aperture comparable to the SPT beam size. We demonstrate the utility of this method to measure YSZ and to constrain mass scaling relations using X-ray mass estimates for a sample of 18 galaxy clusters from the SPT-SZ survey. Measuring YSZ within a 0.75' radius aperture, we find an intrinsic log-normal scatter of 21+/-11% in YSZ at a fixed mass. Measuring YSZ within a 0.3 Mpc projected radius (equivalent to 0.75' at the survey median redshift z = 0.6), we find a scatter of 26+/-9%. Prior to this study, the SPT observable found to have the lowest scatter with mass was cluster detection significance. We demonstrate, from both simulations and SPT observed clusters, that YSZ measured within an aperture comparable to the SPT beam size is equivalent, in terms of scatter with cluster mass, to SPT cluster detection significance.
Published: 2015

6. GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY

Author: Bleem, LE, Stalder, B, de Haan, T, Aird, KA, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hoekstra, H, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Bleem, LE, Stalder, B, de Haan, T, Aird, KA, Allen, SW, Applegate, DE, Ashby, MLN, Bautz, M, Bayliss, M, Benson, BA, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dietrich, JP, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hoekstra, H, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Schrabback, T, Shirokoff, E, Song, J, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: We present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg$^2$ of South Pole Telescope (SPT) data. This work represents the complete sample of clusters detected at high significance in the 2500-square-degree SPT-SZ survey, which was completed in 2011. A total of 677 (409) cluster candidates are identified above a signal-to-noise threshold of $\xi$ =4.5 (5.0). Ground- and space-based optical and near-infrared (NIR) imaging confirms overdensities of similarly colored galaxies in the direction of 516 (or 76%) of the $\xi$>4.5 candidates and 387 (or 95%) of the $\xi$>5 candidates; the measured purity is consistent with expectations from simulations. Of these confirmed clusters, 415 were first identified in SPT data, including 251 new discoveries reported in this work. We estimate photometric redshifts for all candidates with identified optical and/or NIR counterparts; we additionally report redshifts derived from spectroscopic observations for 141 of these systems. The mass threshold of the catalog is roughly independent of redshift above $z$~0.25 leading to a sample of massive clusters that extends to high redshift. The median mass of the sample is $M_{\scriptsize 500c}(\rho_\mathrm{crit})$ ~ 3.5 x 10$^{14} M_\odot h^{-1}$, the median redshift is $z_{med}$ =0.55, and the highest-redshift systems are at $z$>1.4. The combination of large redshift extent, clean selection, and high typical mass makes this cluster sample of particular interest for cosmological analyses and studies of cluster formation and evolution.
Published: 2015

7. A MEASUREMENT OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES FROM THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

Author: George, EM, Reichardt, CL, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, Halverson, NW, Harrington, NL, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mocanu, LM, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, George, EM, Reichardt, CL, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, Halverson, NW, Harrington, NL, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mocanu, LM, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Abstract: We present measurements of secondary cosmic microwave background (CMB) anisotropies and cosmic infrared background (CIB) fluctuations using data from the South Pole Telescope (SPT) covering the complete 2540 sq.deg. SPT-SZ survey area. Data in the three SPT-SZ frequency bands centered at 95, 150, and 220 GHz, are used to produce six angular power spectra (three single-frequency auto-spectra and three cross-spectra) covering the multipole range 2000 < ell < 11000 (angular scales 5' > \theta > 1'). These are the most precise measurements of the angular power spectra at ell > 2500 at these frequencies. The main contributors to the power spectra at these angular scales and frequencies are the primary CMB, CIB, thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ), and radio galaxies. We include a constraint on the tSZ power from a measurement of the tSZ bispectrum from 800 sq.deg. of the SPT-SZ survey. We measure the tSZ power at 143 GHz to be DtSZ = 4.08 +0.58 -0.67 \mu K^2 and the kSZ power to be DkSZ = 2.9 +- 1.3 \mu K^2. The data prefer positive kSZ power at 98.1% CL. We measure a correlation coefficient of \xi = 0.113 +0.057 -0.054 between sources of tSZ and CIB power, with \xi < 0 disfavored at a confidence level of 99.0%. The constraint on kSZ power can be interpreted as an upper limit on the duration of reionization. When the post-reionization homogeneous kSZ signal is accounted for, we find an upper limit on the duration \Delta z < 5.4 at 95% CL.
Published: 2015

8. Optical Spectroscopy and Velocity Dispersions of Galaxy Clusters from the SPT-SZ Survey

Author: Ruel, J, Bazin, G, Bayliss, M, Brodwin, M, Foley, RJ, Stalder, B, Aird, KA, Armstrong, R, Ashby, MLN, Bautz, M, Benson, BA, Bleem, LE, Bocquet, S, Carlstrom, JE, Chang, CL, Chapman, SC, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Nurgaliev, D, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, v Suhada, R, Spieler, HG, Stanford, SA, Staniszewski, Z, Starsk, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Ruel, J, Bazin, G, Bayliss, M, Brodwin, M, Foley, RJ, Stalder, B, Aird, KA, Armstrong, R, Ashby, MLN, Bautz, M, Benson, BA, Bleem, LE, Bocquet, S, Carlstrom, JE, Chang, CL, Chapman, SC, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Nurgaliev, D, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, v Suhada, R, Spieler, HG, Stanford, SA, Staniszewski, Z, Starsk, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: We present optical spectroscopy of galaxies in clusters detected through the Sunyaev-Zel'dovich (SZ) effect with the South Pole Telescope (SPT). We report our own measurements of $61$ spectroscopic cluster redshifts, and $48$ velocity dispersions each calculated with more than $15$ member galaxies. This catalog also includes $19$ dispersions of SPT-observed clusters previously reported in the literature. The majority of the clusters in this paper are SPT-discovered; of these, most have been previously reported in other SPT cluster catalogs, and five are reported here as SPT discoveries for the first time. By performing a resampling analysis of galaxy velocities, we find that unbiased velocity dispersions can be obtained from a relatively small number of member galaxies ($\lesssim 30$), but with increased systematic scatter. We use this analysis to determine statistical confidence intervals that include the effect of membership selection. We fit scaling relations between the observed cluster velocity dispersions and mass estimates from SZ and X-ray observables. In both cases, the results are consistent with the scaling relation between velocity dispersion and mass expected from dark-matter simulations. We measure a $\sim$30% log-normal scatter in dispersion at fixed mass, and a $\sim$10% offset in the normalization of the dispersion-mass relation when compared to the expectation from simulations, which is within the expected level of systematic uncertainty.
Published: 2014

9. A MEASUREMENT OF THE SECONDARY-CMB AND MILLIMETER-WAVE-FOREGROUND BISPECTRUM USING 800 deg2 OF SOUTH POLE TELESCOPE DATA

Author: Crawford, TM, Schaffer, KK, Bhattacharya, S, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hou, Z, Hrubes, JD, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mocanu, LM, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Ruhl, JE, Sayre, JT, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Crawford, TM, Schaffer, KK, Bhattacharya, S, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hou, Z, Hrubes, JD, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mocanu, LM, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Ruhl, JE, Sayre, JT, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, KT, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Abstract: We present a measurement of the angular bispectrum of the millimeter-wave sky in observing bands centered at roughly 95, 150, and 220 GHz, on angular scales of $1^\prime \lesssim \theta \lesssim 10^\prime$ (multipole number $1000 \lesssim l \lesssim 10000$). At these frequencies and angular scales, the main contributions to the bispectrum are expected to be the thermal Sunyaev-Zel'dovich (tSZ) effect and emission from extragalactic sources, predominantly dusty, star-forming galaxies (DSFGs) and active galactic nuclei. We measure the bispectrum in 800 $\mathrm{deg}^2$ of three-band South Pole Telescope data, and we use a multi-frequency fitting procedure to separate the bispectrum of the tSZ effect from the extragalactic source contribution. We simultaneously detect the bispectrum of the tSZ effect at $>$10$\sigma$, the unclustered component of the extragalactic source bispectrum at $>$5$\sigma$ in each frequency band, and the bispectrum due to the clustering of DSFGs---i.e., the clustered cosmic infrared background (CIB) bispectrum---at $>$5$\sigma$. This is the first reported detection of the clustered CIB bispectrum. We use the measured tSZ bispectrum amplitude, compared to model predictions, to constrain the normalization of the matter power spectrum to be $\sigma_8 = 0.787 \pm 0.031$ and to predict the amplitude of the tSZ power spectrum at $l = 3000$. This prediction improves our ability to separate the thermal and kinematic contributions to the total SZ power spectrum. The addition of bispectrum data improves our constraint on the tSZ power spectrum amplitude by a factor of two compared to power spectrum measurements alone and demonstrates a preference for a nonzero kinematic SZ (kSZ) power spectrum, with a derived constraint on the kSZ amplitude at $l=3000$ of A_kSZ $ = 2.9 \pm 1.6 \ \mu$K$^2$, or A_kSZ $ = 2.6 \pm 1.8 \ \mu$K$^2$ if the default A_kSZ > 0 prior is removed.
Published: 2014

10. THE REDSHIFT EVOLUTION OF THE MEAN TEMPERATURE, PRESSURE, AND ENTROPY PROFILES IN 80 SPT-SELECTED GALAXY CLUSTERS

Author: McDonald, M, Benson, BA, Vikhlinin, A, Aird, KA, Allen, SW, Bautz, M, Bayliss, M, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McMahon, JJ, Meyer, SS, Miller, ED, Mocanu, L, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Zenteno, A, McDonald, M, Benson, BA, Vikhlinin, A, Aird, KA, Allen, SW, Bautz, M, Bayliss, M, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hlavacek-Larrondo, J, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McMahon, JJ, Meyer, SS, Miller, ED, Mocanu, L, Mohr, JJ, Murray, SS, Padin, S, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Stanford, SA, Staniszewski, Z, Stark, AA, Story, KT, Stubbs, CW, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, and Zenteno, A
Published: 2014

11. Constraints on the CMB temperature evolution using multiband measurements of the Sunyaev-Zel'dovich effect with the South Pole Telescope

Author: Saro, A, Liu, J, Mohr, JJ, Aird, KA, Ashby, MLN, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Dolag, K, Dudley, JP, Foley, RJ, Gangkofner, D, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hlavacek-Larrondo, J, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Montroy, TE, Murray, SS, Nurgaliev, D, Padin, S, Patej, A, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Saro, A, Liu, J, Mohr, JJ, Aird, KA, Ashby, MLN, Bayliss, M, Benson, BA, Bleem, LE, Bocquet, S, Brodwin, M, Carlstrom, JE, Chang, CL, Chiu, I, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Dolag, K, Dudley, JP, Foley, RJ, Gangkofner, D, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Hennig, C, Hlavacek-Larrondo, J, Holzapfel, WL, Hrubes, JD, Jones, C, Keisler, R, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Montroy, TE, Murray, SS, Nurgaliev, D, Padin, S, Patej, A, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: The adiabatic evolution of the temperature of the cosmic microwave background (CMB) is a key prediction of standard cosmology. We study deviations from the expected adiabatic evolution of the CMB temperature of the form $T(z) =T_0(1+z)^{1-\alpha}$ using measurements of the spectrum of the Sunyaev Zel'dovich Effect with the South Pole Telescope (SPT). We present a method for using the ratio of the Sunyaev Zel'dovich signal measured at 95 and 150 GHz in the SPT data to constrain the temperature of the CMB. We demonstrate that this approach provides unbiased results using mock observations of clusters from a new set of hydrodynamical simulations. We apply this method to a sample of 158 SPT-selected clusters, spanning the redshift range $0.05 < z < 1.35$, and measure $\alpha = 0.017^{+0.030}_{-0.028}$, consistent with the standard model prediction of $\alpha=0$. In combination with other published results, we constrain $\alpha = 0.011 \pm 0.016$, an improvement of $\sim 20\%$ over published constraints. This measurement also provides a strong constraint on the effective equation of state in models of decaying dark energy $w_\mathrm{eff} = -0.987^{+0.016}_{-0.017}$.
Published: 2014

12. SPT-CL J2040-4451: AN SZ-SELECTED GALAXY CLUSTER AT z=1.478 WITH SIGNIFICANT ONGOING STAR FORMATION

Author: Bayliss, MB, Ashby, MLN, Ruel, J, Brodwin, M, Aird, KA, Bautz, MW, Benson, BA, Bleem, LE, Bocquet, S, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiattii, A, Crawford, TM, Crites, AT, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gettings, D, Gladders, MD, Gonzalez, AH, de Haan, T, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, Mawatari, K, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Miller, ED, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Song, J, Stalder, B, Suhada, R, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, R, Zenteno, A, Bayliss, MB, Ashby, MLN, Ruel, J, Brodwin, M, Aird, KA, Bautz, MW, Benson, BA, Bleem, LE, Bocquet, S, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiattii, A, Crawford, TM, Crites, AT, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gettings, D, Gladders, MD, Gonzalez, AH, de Haan, T, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, Mawatari, K, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Miller, ED, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shirokoff, E, Song, J, Stalder, B, Suhada, R, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, R, and Zenteno, A
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.
Published: 2014

13. CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg2 SPT-SZ SURVEY

Author: Hou, Z, Reichardt, CL, Story, KT, Follin, B, Keisler, R, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, De Haan, T, De Putter, R, Dobbs, MA, Dodelson, S, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Joy, M, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Hou, Z, Reichardt, CL, Story, KT, Follin, B, Keisler, R, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, De Haan, T, De Putter, R, Dobbs, MA, Dodelson, S, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Joy, M, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Published: 2014

14. SPT-CL J0205-5829: A z=1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY

Author: Stalder, B, Ruel, J, Suhada, R, Brodwin, M, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gettings, D, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Nurgaliev, D, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Stalder, B, Ruel, J, Suhada, R, Brodwin, M, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gettings, D, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Nurgaliev, D, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stanford, SA, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: The galaxy cluster SPT-CL J0205-5829 currently has the highest spectroscopically-confirmed redshift, z=1.322, in the South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey. XMM-Newton observations measure a core-excluded temperature of Tx=8.7keV producing a mass estimate that is consistent with the Sunyaev-Zel'dovich derived mass. The combined SZ and X-ray mass estimate of M500=(4.9+/-0.8)e14 h_{70}^{-1} Msun makes it the most massive known SZ-selected galaxy cluster at z>1.2 and the second most massive at z>1. Using optical and infrared observations, we find that the brightest galaxies in SPT-CL J0205-5829 are already well evolved by the time the universe was <5 Gyr old, with stellar population ages >3 Gyr, and low rates of star formation (<0.5Msun/yr). We find that, despite the high redshift and mass, the existence of SPT-CL J0205-5829 is not surprising given a flat LambdaCDM cosmology with Gaussian initial perturbations. The a priori chance of finding a cluster of similar rarity (or rarer) in a survey the size of the 2500 deg^2 SPT-SZ survey is 69%.
Published: 2013

15. COSMOLOGICAL CONSTRAINTS FROM SUNYAEV-ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg2 OF THE SOUTH POLE TELESCOPE SURVEY

Author: Benson, BA, de Haan, T, Dudley, JP, Reichardt, CL, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, N, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Padin, S, Plagge, T, Pryke, C, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Suhada, R, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Benson, BA, de Haan, T, Dudley, JP, Reichardt, CL, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, Desai, S, Dobbs, MA, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, N, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Montroy, TE, Murray, SS, Natoli, T, Padin, S, Plagge, T, Pryke, C, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Suhada, R, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: We use measurements from the South Pole Telescope (SPT) Sunyaev Zel'dovich (SZ) cluster survey in combination with X-ray measurements to constrain cosmological parameters. We present a statistical method that fits for the scaling relations of the SZ and X-ray cluster observables with mass while jointly fitting for cosmology. The method is generalizable to multiple cluster observables, and self-consistently accounts for the effects of the cluster selection and uncertainties in cluster mass calibration on the derived cosmological constraints. We apply this method to a data set consisting of an SZ-selected catalog of 18 galaxy clusters at z > 0.3 from the first 178 deg2 of the 2500 deg2 SPT-SZ survey, with 14 clusters having X-ray observations from either Chandra or XMM. Assuming a spatially flat LCDM cosmological model, we find the SPT cluster sample constrain sigma_8 (Omega_m/0.25)^0.30 = 0.785 +- 0.037. In combination with measurements of the CMB power spectrum from the SPT and the seven-year WMAP data, the SPT cluster sample constrain sigma_8 = 0.795 +- 0.016 and Omega_m = 0.255 +- 0.016, a factor of 1.5 improvement on each parameter over the CMB data alone. We consider several extensions beyond the LCDM model by including the following as free parameters: the dark energy equation of state (w), the sum of the neutrino masses (sum mnu), the effective number of relativistic species (Neff), and a primordial non-Gaussianity (fNL). We find that adding the SPT cluster data significantly improves the constraints on w and sum mnu beyond those found when using measurements of the CMB, supernovae, baryon acoustic oscillations, and the Hubble constant. Considering each extension independently, we best constrain w=-0.973 +- 0.063 and the sum of neutrino masses sum mnu < 0.28 eV at 95% confidence, a factor of 1.25 and 1.4 improvement, respectively, over the constraints without clusters. [abbrev.]
Published: 2013

16. GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY

Author: Reichardt, CL, Stalder, B, Bleem, LE, Montroy, TE, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Benson, BA, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Natoli, T, Padin, S, Plagge, T, Pryke, C, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Suhada, R, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, Zenteno, A, Reichardt, CL, Stalder, B, Bleem, LE, Montroy, TE, Aird, KA, Andersson, K, Armstrong, R, Ashby, MLN, Bautz, M, Bayliss, M, Bazin, G, Benson, BA, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, HM, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, Harrington, NL, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Liu, J, Lueker, M, Luong-Van, D, Mantz, A, Marrone, DP, McDonald, M, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Mohr, JJ, Murray, SS, Natoli, T, Padin, S, Plagge, T, Pryke, C, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Sayre, JT, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, Stubbs, CW, Suhada, R, van Engelen, A, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Zahn, O, and Zenteno, A
Abstract: We present a catalog of 224 galaxy cluster candidates, selected through their Sunyaev-Zel'dovich (SZ) effect signature in the first 720 deg2 of the South Pole Telescope (SPT) survey. This area was mapped with the SPT in the 2008 and 2009 austral winters to a depth of 18 uK-arcmin at 150 GHz; 550 deg2 of it was also mapped to 44 uK-arcmin at 95 GHz. Based on optical imaging of all candidates and near-infrared imaging of the majority of candidates, we have found optical and/or infrared counterparts for 158 clusters. Of these, 135 were first identified as clusters in SPT data, including 117 new discoveries reported in this work. This catalog triples the number of confirmed galaxy clusters discovered through the SZ effect. We report photometrically derived (and in some cases spectroscopic) redshifts for confirmed clusters and redshift lower limits for the remaining candidates. The catalog extends to high redshift with a median redshift of z = 0.55 and maximum redshift of z = 1.37. Based on simulations, we expect the catalog to be nearly 100% complete above M500 ~ 5e14 Msun h_{70}^-1 at z > 0.6. There are 121 candidates detected at signal-to-noise greater than five, at which the catalog purity is measured to be 95%. From this high-purity subsample, we exclude the z < 0.3 clusters and use the remaining 100 candidates to improve cosmological constraints following the method presented by Benson et al., 2011. Adding the cluster data to CMB+BAO+H0 data leads to a preference for non-zero neutrino masses while only slightly reducing the upper limit on the sum of neutrino masses to sum mnu < 0.38 eV (95% CL). For a spatially flat wCDM cosmological model, the addition of this catalog to the CMB+BAO+H0+SNe results yields sigma8=0.807+-0.027 and w = -1.010+-0.058, improving the constraints on these parameters by a factor of 1.4 and 1.3, respectively. [abbrev]
Published: 2013

17. IMPROVED CONSTRAINTS ON COSMIC MICROWAVE BACKGROUND SECONDARY ANISOTROPIES FROM THE COMPLETE 2008 SOUTH POLE TELESCOPE DATA

Author: Shirokoff, E, Reichardt, CL, Shaw, L, Millea, M, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Shirokoff, E, Reichardt, CL, Shaw, L, Millea, M, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Abstract: We report measurements of the cosmic microwave background (CMB) power spectrum from the complete 2008 South Pole Telescope (SPT) data set. We analyze twice as much data as the first SPT power spectrum analysis, using an improved cosmological parameter estimator which fits multi-frequency models to the SPT 150 and $220\,$GHz bandpowers. We find an excellent fit to the measured bandpowers with a model that includes lensed primary CMB anisotropy, secondary thermal (tSZ) and kinetic (kSZ) Sunyaev-Zel'dovich anisotropies, unclustered synchrotron point sources, and clustered dusty point sources. In addition to measuring the power spectrum of dusty galaxies at high signal-to-noise, the data primarily constrain a linear combination of the kSZ and tSZ anisotropy contributions at $150\,$GHz and $\ell=3000$: $D^{tSZ}_{3000} + 0.5\,D^{kSZ}_{3000} = 4.5\pm 1.0 \,\mu{\rm K}^2$. The 95% confidence upper limits on secondary anisotropy power are $D^{tSZ}_{3000} < 5.3\,\mu{\rm K}^2$ and $D^{kSZ}_{3000} < 6.5\,\mu{\rm K}^2$. We also consider the potential correlation of dusty and tSZ sources, and find it incapable of relaxing the tSZ upper limit. These results increase the significance of the lower than expected tSZ amplitude previously determined from SPT power spectrum measurements. We find that models including non-thermal pressure support in groups and clusters predict tSZ power in better agreement with the SPT data. Combining the tSZ power measurement with primary CMB data halves the statistical uncertainty on $\sigma_8$. However, the preferred value of $\sigma_8$ varies significantly between tSZ models. Improved constraints on cosmological parameters from tSZ power spectrum measurements require continued progress in the modeling of the tSZ power.
Published: 2011

18. X-RAY PROPERTIES OF THE FIRST SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTER SAMPLE FROM THE SOUTH POLE TELESCOPE

Author: Andersson, K, Benson, BA, Ade, PAR, Aird, KA, Armstrong, B, Bautz, M, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, Garmire, G, George, EM, Gladders, MD, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Murray, SS, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Yang, Y, Zahn, O, Zenteno, A, Andersson, K, Benson, BA, Ade, PAR, Aird, KA, Armstrong, B, Bautz, M, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, Forman, WR, Garmire, G, George, EM, Gladders, MD, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Jones, C, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Murray, SS, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, Vanderlinde, K, Vieira, JD, Vikhlinin, A, Williamson, R, Yang, Y, Zahn, O, and Zenteno, A
Abstract: We present results of X-ray observations of a sample of 15 clusters selected via their imprint on the cosmic microwave background (CMB) from the thermal Sunyaev-Zel'dovich (SZ) effect. These clusters are a subset of the first SZ-selected cluster catalog, obtained from observations of 178 deg^2 of sky surveyed by the South Pole Telescope. Using X-ray observations with Chandra and XMM-Newton, we estimate the temperature, T_X, and mass, M_g, of the intracluster medium (ICM) within r_500 for each cluster. From these, we calculate Y_X=M_g T_X and estimate the total cluster mass using a M_500-Y_X scaling relation measured from previous X-ray studies. The integrated Comptonization, Y_SZ, is derived from the SZ measurements, using additional information from the X-ray measured gas density profiles and a universal temperature profile. We calculate scaling relations between the X-ray and SZ observables, and find results generally consistent with other measurements and the expectations from simple self-similar behavior. Specifically, we fit a Y_SZ-Y_X relation and find a normalization of 0.82 +- 0.07, marginally consistent with the predicted ratio of Y_SZ/Y_X=0.91+-0.01 that would be expected from the density and temperature models used in this work. Using the Y_X derived mass estimates, we fit a Y_SZ-M_500 relation and find a slope consistent with the self-similar expectation of Y_SZ ~ M^5/3 with a normalization consistent with predictions from other X-ray studies. We compare the X-ray mass estimates to previously published SZ mass estimates derived from cosmological simulations of the SPT survey. We find that the SZ mass estimates are lower by a factor of 0.89+-0.06, which is within the ~15% systematic uncertainty quoted for the simulation-based SZ masses.
Published: 2011

19. SOUTH POLE TELESCOPE DETECTIONS OF THE PREVIOUSLY UNCONFIRMED PLANCK EARLY SUNYAEV-ZEL'DOVICH CLUSTERS IN THE SOUTHERN HEMISPHERE

Author: Story, K, Aird, KA, Andersson, K, Armstrong, R, Bazin, G, Benson, BA, Bleem, LE, Bonamente, M, Brodwin, M, Carlstrom, JE, Chang, CL, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, Vanderlinde, K, Vieira, JD, Williamson, R, Zenteno, A, Story, K, Aird, KA, Andersson, K, Armstrong, R, Bazin, G, Benson, BA, Bleem, LE, Bonamente, M, Brodwin, M, Carlstrom, JE, Chang, CL, Clocchiatti, A, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, George, EM, Gladders, MD, Gonzalez, AH, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hoover, S, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Saliwanchik, BR, Saro, A, Schaffer, KK, Shaw, L, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, Vanderlinde, K, Vieira, JD, Williamson, R, and Zenteno, A
Abstract: We present South Pole Telescope (SPT) observations of the five galaxy cluster candidates in the southern hemisphere which were reported as unconfirmed in the Planck Early Sunyaev-Zel'dovich (ESZ) sample. One cluster candidate, PLCKESZ G255.62-46.16, is located in the 2500-square-degree SPT SZ survey region and was reported previously as SPT-CL J0411-4819. For the remaining four candidates, which are located outside of the SPT SZ survey region, we performed short, dedicated SPT observations. Each of these four candidates was strongly detected in maps made from these observations, with signal-to-noise ratios ranging from 6.3 to 13.8. We have observed these four candidates on the Magellan-Baade telescope and used these data to estimate cluster redshifts from the red sequence. Resulting redshifts range from 0.24 to 0.46. We report measurements of Y_0.75', the integrated Comptonization within a 0.75' radius, for all five candidates. We also report X-ray luminosities calculated from ROSAT All-Sky Survey catalog counts, as well as optical and improved SZ coordinates for each candidate. The combination of SPT SZ measurements, optical red-sequence measurements, and X-ray luminosity estimates demonstrates that these five Planck ESZ cluster candidates do indeed correspond to real galaxy clusters with redshifts and observable properties consistent with the rest of the ESZ sample.
Published: 2011

20. A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE

Author: Keisler, R, Reichardt, CL, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hou, Z, Hrubes, JD, Joy, M, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mohr, JJ, Montroy, TE, Natoli, T, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Keisler, R, Reichardt, CL, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Dudley, J, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hoover, S, Hou, Z, Hrubes, JD, Joy, M, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Millea, M, Mohr, JJ, Montroy, TE, Natoli, T, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Staniszewski, Z, Stark, AA, Story, K, van Engelen, A, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Abstract: We present a measurement of the angular power spectrum of the cosmic microwave background (CMB) using data from the South Pole Telescope (SPT). The data consist of 790 square degrees of sky observed at 150 GHz during 2008 and 2009. Here we present the power spectrum over the multipole range 650 < ell < 3000, where it is dominated by primary CMB anisotropy. We combine this power spectrum with the power spectra from the seven-year Wilkinson Microwave Anisotropy Probe (WMAP) data release to constrain cosmological models. We find that the SPT and WMAP data are consistent with each other and, when combined, are well fit by a spatially flat, LCDM cosmological model. The SPT+WMAP constraint on the spectral index of scalar fluctuations is ns = 0.9663 +/- 0.0112. We detect, at ~5-sigma significance, the effect of gravitational lensing on the CMB power spectrum, and find its amplitude to be consistent with the LCDM cosmological model. We explore a number of extensions beyond the LCDM model. Each extension is tested independently, although there are degeneracies between some of the extension parameters. We constrain the tensor-to-scalar ratio to be r < 0.21 (95% CL) and constrain the running of the scalar spectral index to be dns/dlnk = -0.024 +/- 0.013. We strongly detect the effects of primordial helium and neutrinos on the CMB; a model without helium is rejected at 7.7-sigma, while a model without neutrinos is rejected at 7.5-sigma. The primordial helium abundance is measured to be Yp = 0.296 +/- 0.030, and the effective number of relativistic species is measured to be Neff = 3.85 +/- 0.62. The constraints on these models are strengthened when the CMB data are combined with measurements of the Hubble constant and the baryon acoustic oscillation feature. Notable improvements include ns = 0.9668 +/- 0.0093, r < 0.17 (95% CL), and Neff = 3.86 +/- 0.42. The SPT+WMAP data show...
Published: 2011

21. OPTICAL REDSHIFT AND RICHNESS ESTIMATES FOR GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS

Author: High, FW, Stalder, B, Song, J, Ade, PAR, Aird, KA, Allam, SS, Armstrong, R, Barkhouse, WA, Benson, BA, Bertin, E, Bhattacharya, S, Bleem, LE, Brodwin, M, Buckley-Geer, EJ, Carlstrom, JE, Challis, P, Chang, CL, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, George, EM, Gladders, M, Halverson, NW, Hamuy, M, Hansen, SM, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Lee, AT, Leitch, EM, Lin, H, Lin, Y-T, Loehr, A, Lueker, M, Marrone, D, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Morell, N, Ngeow, C-C, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Smith, RC, Spieler, HG, Staniszewski, Z, Stark, AA, Stubbs, CW, Tucker, DL, Vanderlinde, K, Vieira, JD, Williamson, R, Wood-Vasey, WM, Yang, Y, Zahn, O, Zenteno, A, High, FW, Stalder, B, Song, J, Ade, PAR, Aird, KA, Allam, SS, Armstrong, R, Barkhouse, WA, Benson, BA, Bertin, E, Bhattacharya, S, Bleem, LE, Brodwin, M, Buckley-Geer, EJ, Carlstrom, JE, Challis, P, Chang, CL, Crawford, TM, Crites, AT, de Haan, T, Desai, S, Dobbs, MA, Dudley, JP, Foley, RJ, George, EM, Gladders, M, Halverson, NW, Hamuy, M, Hansen, SM, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Lee, AT, Leitch, EM, Lin, H, Lin, Y-T, Loehr, A, Lueker, M, Marrone, D, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Morell, N, Ngeow, C-C, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Smith, RC, Spieler, HG, Staniszewski, Z, Stark, AA, Stubbs, CW, Tucker, DL, Vanderlinde, K, Vieira, JD, Williamson, R, Wood-Vasey, WM, Yang, Y, Zahn, O, and Zenteno, A
Abstract: We present redshifts and optical richness properties of 21 galaxy clusters uniformly selected by their Sunyaev-Zel'dovich signature. These clusters, plus an additional, unconfirmed candidate, were detected in a 178 square-degree area surveyed by the South Pole Telescope in 2008. Using griz imaging from the Blanco Cosmology Survey and from pointed Magellan telescope observations, as well as spectroscopy using Magellan facilities, we confirm the existence of clustered red-sequence galaxies, report red-sequence photometric redshifts, present spectroscopic redshifts for a subsample, and derive R_200 radii and M_200 masses from optical richness. The clusters span redshifts from 0.15 to greater than 1, with a median redshift of 0.74; three clusters are estimated to be at z > 1. Redshifts inferred from mean red-sequence colors exhibit 2% RMS scatter in sigma_z/(1+z) with respect to the spectroscopic subsample for z < 1. We show that M_200 cluster masses derived from optical richness correlate with masses derived from South Pole Telescope data and agree with previously derived scaling relations to within the uncertainties. Optical and infrared imaging is an efficient means of cluster identification and redshift estimation in large Sunyaev-Zel'dovich surveys, and exploiting the same data for richness measurements, as we have done, will be useful for constraining cluster masses and radii for large samples in cosmological analysis.
Published: 2010

22. EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD

Author: Vieira, JD, Crawford, TM, Switzer, ER, Ade, PAR, Aird, KA, Ashby, MLN, Benson, BA, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, H-M, Crites, AT, de Haan, T, Dobbs, MA, Everett, W, George, EM, Gladders, M, Hall, NR, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Marrone, DP, McIntyre, V, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Vanderlinde, K, Walsh, W, Williamson, R, Yang, Y, Zahn, O, Zenteno, A, Vieira, JD, Crawford, TM, Switzer, ER, Ade, PAR, Aird, KA, Ashby, MLN, Benson, BA, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Cho, H-M, Crites, AT, de Haan, T, Dobbs, MA, Everett, W, George, EM, Gladders, M, Hall, NR, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Lueker, M, Marrone, DP, McIntyre, V, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Vanderlinde, K, Walsh, W, Williamson, R, Yang, Y, Zahn, O, and Zenteno, A
Abstract: We report the results of an 87 square-degree point-source survey centered at R.A. 5h30m, decl. -55 deg. taken with the South Pole Telescope (SPT) at 1.4 and 2.0 mm wavelengths with arc-minute resolution and milli-Jansky depth. Based on the ratio of flux in the two bands, we separate the detected sources into two populations, one consistent with synchrotron emission from active galactic nuclei (AGN) and one consistent with thermal emission from dust. We present source counts for each population from 11 to 640 mJy at 1.4 mm and from 4.4 to 800 mJy at 2.0 mm. The 2.0 mm counts are dominated by synchrotron-dominated sources across our reported flux range; the 1.4 mm counts are dominated by synchroton-dominated sources above ~15 mJy and by dust-dominated sources below that flux level. We detect 141 synchrotron-dominated sources and 47 dust-dominated sources at S/N > 4.5 in at least one band. All of the most significantly detected members of the synchrotron-dominated population are associated with sources in previously published radio catalogs. Some of the dust-dominated sources are associated with nearby (z << 1) galaxies whose dust emission is also detected by the Infrared Astronomy Satellite (IRAS). However, most of the bright, dust-dominated sources have no counterparts in any existing catalogs. We argue that these sources represent the rarest and brightest members of the population commonly referred to as sub-millimeter galaxies (SMGs). Because these sources are selected at longer wavelengths than in typical SMG surveys, they are expected to have a higher mean redshift distribution and may provide a new window on galaxy formation in the early universe.
Published: 2010

23. MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE

Author: Lueker, M, Reichardt, CL, Schaffer, KK, Zahn, O, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, George, EM, Hall, NR, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Vanderlinde, K, Vieira, JD, Williamson, R, Lueker, M, Reichardt, CL, Schaffer, KK, Zahn, O, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, George, EM, Hall, NR, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Vanderlinde, K, Vieira, JD, and Williamson, R
Abstract: We report cosmic microwave background (CMB) power spectrum measurements from the first 100 sq. deg. field observed by the South Pole Telescope (SPT) at 150 and 220 GHz. On angular scales where the primary CMB anisotropy is dominant, ell ~< 3000, the SPT power spectrum is consistent with the standard LambdaCDM cosmology. On smaller scales, we see strong evidence for a point source contribution, consistent with a population of dusty, star-forming galaxies. After we mask bright point sources, anisotropy power on angular scales of 3000 < ell < 9500 is detected with a signal-to-noise > 50 at both frequencies. We combine the 150 and 220 GHz data to remove the majority of the point source power, and use the point source subtracted spectrum to detect Sunyaev-Zel'dovich (SZ) power at 2.6 sigma. At ell=3000, the SZ power in the subtracted bandpowers is 4.2 +/- 1.5 uK^2, which is significantly lower than the power predicted by a fiducial model using WMAP5 cosmological parameters. This discrepancy may suggest that contemporary galaxy cluster models overestimate the thermal pressure of intracluster gas. Alternatively, this result can be interpreted as evidence for lower values of sigma8. When combined with an estimate of the kinetic SZ contribution, the measured SZ amplitude shifts sigma8 from the primary CMB anisotropy derived constraint of 0.794 +/- 0.028 down to 0.773 +/- 0.025. The uncertainty in the constraint on sigma8 from this analysis is dominated by uncertainties in the theoretical modeling required to predict the amplitude of the SZ power spectrum for a given set of cosmological parameters.
Published: 2010

24. ANGULAR POWER SPECTRA OF THE MILLIMETER-WAVELENGTH BACKGROUND LIGHT FROM DUSTY STAR-FORMING GALAXIES WITH THE SOUTH POLE TELESCOPE

Author: Hall, NR, Keisler, R, Knox, L, Reichardt, CL, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, De Haan, T, Dobbs, MA, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Lee, AT, Leitch, EM, Lueker, M, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Switzer, ER, Vanderlinde, K, Vieira, JD, Williamson, R, Zahn, O, Hall, NR, Keisler, R, Knox, L, Reichardt, CL, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, H-M, Crawford, TM, Crites, AT, De Haan, T, Dobbs, MA, George, EM, Halverson, NW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Lee, AT, Leitch, EM, Lueker, M, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Padin, S, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Switzer, ER, Vanderlinde, K, Vieira, JD, Williamson, R, and Zahn, O
Abstract: We use data from the first 100 square-degree field observed by the South Pole Telescope (SPT) in 2008 to measure the angular power spectrum of temperature anisotropies contributed by the background of dusty star-forming galaxies (DSFGs) at millimeter wavelengths. From the auto and cross-correlation of 150 and 220 GHz SPT maps, we significantly detect both Poisson distributed and, for the first time at millimeter wavelengths, clustered components of power from a background of DSFGs. The spectral indices between 150 and 220 GHz of the Poisson and clustered components are found to be 3.86 +- 0.23 and 3.8 +- 1.3 respectively, implying a steep scaling of the dust emissivity index beta ~ 2. The Poisson and clustered power detected in SPT, BLAST (at 600, 860, and 1200 GHz), and Spitzer (1900 GHz) data can be understood in the context of a simple model in which all galaxies have the same graybody spectrum with dust emissivity index of beta = 2 and dust temperature T_d = 34 K. In this model, half of the 150 GHz background light comes from redshifts greater than 3.2. We also use the SPT data to place an upper limit on the amplitude of the kinetic Sunyaev-Zel'dovich power spectrum at l = 3000 of 13 uK^2 at 95% confidence.
Published: 2010

25. GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS

Author: Vanderlinde, K, Crawford, TM, de Haan, T, Dudley, JP, Shaw, L, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Crites, AT, Desai, S, Dobbs, MA, Foley, RJ, George, EM, Gladders, MD, Hall, NR, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Loehr, A, Lueker, M, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Ngeow, C-C, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, van Engelen, A, Vieira, JD, Williamson, R, Yang, Y, Zahn, O, Zenteno, A, Vanderlinde, K, Crawford, TM, de Haan, T, Dudley, JP, Shaw, L, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Brodwin, M, Carlstrom, JE, Chang, CL, Crites, AT, Desai, S, Dobbs, MA, Foley, RJ, George, EM, Gladders, MD, Hall, NR, Halverson, NW, High, FW, Holder, GP, Holzapfel, WL, Hrubes, JD, Joy, M, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Loehr, A, Lueker, M, Marrone, DP, McMahon, JJ, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Ngeow, C-C, Padin, S, Plagge, T, Pryke, C, Reichardt, CL, Rest, A, Ruel, J, Ruhl, JE, Schaffer, KK, Shirokoff, E, Song, J, Spieler, HG, Stalder, B, Staniszewski, Z, Stark, AA, Stubbs, CW, van Engelen, A, Vieira, JD, Williamson, R, Yang, Y, Zahn, O, and Zenteno, A
Abstract: We present a detection-significance-limited catalog of 21 Sunyaev-Zel'dovich selected galaxy clusters. These clusters, along with 1 unconfirmed candidate, were identified in 178 deg^2 of sky surveyed in 2008 by the South Pole Telescope to a depth of 18 uK-arcmin at 150 GHz. Optical imaging from the Blanco Cosmology Survey (BCS) and Magellan telescopes provided photometric (and in some cases spectroscopic) redshift estimates, with catalog redshifts ranging from z=0.15 to z>1, with a median z = 0.74. Of the 21 confirmed galaxy clusters, three were previously identified as Abell clusters, three were presented as SPT discoveries in Staniszewski et al, 2009, and three were first identified in a recent analysis of BCS data by Menanteau et al, 2010; the remaining 12 clusters are presented for the first time in this work. Simulated observations of the SPT fields predict the sample to be nearly 100% complete above a mass threshold of M_200 ~ 5x10^14 M_sun/h at z = 0.6. This completeness threshold pushes to lower mass with increasing redshift, dropping to ~4x10^14 M_sun/h at z=1. The size and redshift distribution of this catalog are in good agreement with expectations based on our current understanding of galaxy clusters and cosmology. In combination with other cosmological probes, we use the cluster catalog to improve estimates of cosmological parameters. Assuming a standard spatially flat wCDM cosmological model, the addition of our catalog to the WMAP 7-year analysis yields sigma_8 = 0.81 +- 0.09 and w = -1.07 +- 0.29, a ~50% improvement in precision on both parameters over WMAP7 alone.
Published: 2010

26. Letter of Intent by the Solenoidal Detector Collaboration to construct and operate a detector at the Superconducting Super Collider

Author: SDC Collaboration, Trilling, GH, Berger, EL, Blair, RE, Dawson, JW, Ekenberg, TL, Derrick, M, Fields, TH, Guarino, V, Hagstrom, RT, Hill, NF, Job, P, Kirk, TBW, May, EN, Nasiatka, J, Nodulman, LJ, Price, LE, Proudfoot, J, Spinka, HM, Talaga, RL, Trost, HJ, Underwood, DG, Wagner, RG, Wicklund, AB, Wu, MM, Johns, KA, Cui, Hua-chuan, Gao, Wen-xiu, Huang, De-qiang, Li, Wei-guo, Mao, Hui-shun, Ni, Hui-ling, Qi, Na-ding, Wang, Tai-jie, Yan, Wu-guang, Ye, Ming-han, Zhao, Wei-ren, Zheng, Liu-sheng, Zhou, Yue-hua, Ming, He Yu, Xi, Lai Chu, Tao, Liu Hong, Qiu, Liu Song, Qiao, Lou Bing, Xiang, Yang Ji, De, Yao Shu, Ju, Zhang Re, Behrends, S, Bensinger, JR, Blocker, C, Kesten, P, Kirsch, L, Povinec, P, Strmen, P, Foster, B, Heath, GP, Cutts, D, Gao, GS, Partridge, R, Alexa, A, Horoi, M, Pantea, D, Pentia, M, Petrascu, C, Weinstein, AJ, Gunion, JF, Pellett, D, Mani, S, Lankford, A, Arisaka, K, Bengtsson, HU, Buchanan, C, Chrisman, D, Cline, D, Hauser, J, Muller, T, Park, J, Roberts, D, Slater, W, Ellison, J, Wimpenny, SJ, Sivertz, M, Thomas, D, DeWitt, J, Dorfan, D, Heusch, C, Hubbard, B, Hutchinson, D, Litke, AL, Lockman, WS, Nilsson, W, O'Shaughnessy, K, Pitzl, D, Rowe, W, Sadrozinski, H, Seiden, A, Spencer, E, Armitage, J, Dixit, MS, Estabrooks, P, Godfrey, S, Losty, M, Mes, H, Oakham, G, O'Neille, M, Kawai, H, Campagneri, C, Contreras, M, Eno, S, Frisch, H, Gross-Pilcher, C, Miller, M, Rosenberg, L, Sanders, H, Shochet, M, Sullivan, G, Baranko, GJ, Cheung, HWK, Cumalat, JP, Erdos, E, Ford, WT, Nauenberg, U, Rankin, P, Schultz, G, Smith, JG, Astakhov, VI, Batyunya, BV, Bischoff, A, Budagov, YA, Chuenko, AM, Dokshin, AI, Finger, M, Gerasimov, SB, Golovatyuk, VM, Gotra, Yu N, Gusar, Yu S, Guzik, Z, Khubua, DI, Ilyin, Yu V, Kashigin, SV, Kharzheev, YN, Kolpakov, IF, Kovalenko, AD, Levchanovsky, FV, Lomakin, YF, Malakhov, AI, Matyushevsky, EA, Omelyanenko, AA, Pakhmutov, Yu S, Panebratsev, YA, Puzynin, IV, Semenov, AA, Senner, AE, Shabunov, AV, Sidorov, VT, Sinaev, AN, Sisakian, AN, Smirnov, V, Spassov, T, Tsyganov, EN, Tyapkin, IA, Vasilev, LA, Velev, GV, Vinogradov, VB, Vodopyanov, AS, Vrba, V, Zanevsky, Yu V, Zhuravlev, NI, Zimin, NI, Zinchenko, AI, Goshaw, AT, Oh, SH, Phillips, TJ, Robertson, WJ, Simpkins, JD, Walker, WD, Amatuni, AC, Vartapetian, GA, Areti, VH, Atac, M, Barsotti, E, Bartoszek, L, Baumbaugh, AE, Beretvas, A, Bernstein, R, Binkley, M, Bross, AD, Clark, AG, Cooper, JW, Denby, BH, Denisenko, KG, Denisenko, NL, Droege, T, Eartly, DP, Elias, JE, Fast, RW, Finley, D, Foster, GW, Freeman, J, Gaines, I, Gourlay, SA, Green, DR, Grimson, J, Grozis, C, Hahn, SR, Harris, RM, Hoff, J, Huth, J, Hylen, J, Kephart, RD, Kilmer, J, Krebs, HJ, Kuzminski, J, Lee, A, Limon, PJ, Martin, PS, Mukerjee, A, Nash, T, Newman-Holmes, C, Para, A, Patrick, J, Plunkett, R, Schmidt, EE, Segler, SL, Stanek, RP, Srefanik, A, Stredde, HJ, Tkaczyk, S, Vidal, R, Wagner, RL, Wands, RH, Yarema, R, Yeh, GP, Yoh, J, Zimmerman, T, Field, R, Harmon, J, Walker, J, Corden, M, Hagopian, V, Johnson, K, Wahl, H, Kawaguchi, M, Yoshida, H, Dvornik, AM, Maksimenko, NB, Brandenburg, G, Feldman, G, Franklin, M, Geer, S, Konigsberg, J, Oliver, J, Sadowski, E, Schlabach, P, Wilson, R, Kenney, C, Parker, S, Chiba, Y, Ohsugi, T, Asai, M, Shioden, M, Goldberg, H, Margulies, S, Solomon, J, Downing, R, Errede, S, Gautier, A, Haney, M, Holloway, L, Karliner, I, Liss, A, O'Halloran, T, Thaler, J, Sheldon, P, Simaitis, V, Wiss, J, Blockus, D, Brabson, B, Dzierba, A, Foster, R, Hanson, G, Lou, X, Luehring, F, Martin, B, Ogren, H, Rust, D, Wente, E, Hauptman, J, Bagger, JA, Barnett, BA, Blumenfeld, BJ, Fisher, PH, Matthews, JAJ, Abe, F, Amako, K, Arai, Y, Doi, Y, Fujii, H, Fukui, Y, Haruyama, T, Ikeda, H, Inaba, S, Inagaki, T, Iwasaki, H, Kabe, S, Kanematsu, N, Kanzaki, J, Kondo, T, Maki, A, Manabe, A, Mishina, M, Noumachi, M, Odaka, S, Ogawa, K, Ohska, TK, Sakai, Y, Sakamoto, H, Sasaki, O, Shinkawa, T, Takaiwa, Y, Terada, S, Tsuboyama, T, Tsukada, K, Ujiie, N, Unno, Y, Watase, Y, Yamamoto, A, Yasu, Y, Krivan, F, Seman, M, Spalek, J, Kikuchi, R, Miyake, K, Abrams, GS, Barbaro-Galtieri, A, Barnett, RM, Cahn, RN, Corradi, CA, Eberhard, PH, Einsweiler, K, Edwards, WR, Ely, R, Gilchriese, MGD, Groom, DE, Haber, C, Hearty, C, Hinchliffe, I, Hoff, M, Jared, R, Kadel, RW, Kadyk, JA, Kleinfelder, S, Levi, ME, Lim, A, Loken, SC, Madden, N, Minamihara, YY, Milgrome, O, Millaud, J, Moore, TL, Nygren, DR, Palounek, APT, Pope, WL, Pripstein, M, Rasson, J, Shapiro, M, Shuman, D, Spieler, HG, Stone, R, Strovink, M, Thur, W, Weidenbach, RC, Wenzel, WA, Ziock, H, Bailey, J, Beck, GA, Dainton, JB, Gabathuler, E, Maxfield, SJ, Smith, G, Baden, AR, Ball, AH, Chang, CY, Fong, DG, Goodman, JA, Hadley, NJ, Jawahery, A, Kellogg, RG, Kunori, S, Skuja, A, Zorn, GT, Ragan, K, Stairs, DG, Amidei, D, Ball, RC, Campbell, M, Chapman, J, De, K, Derwent, P, Gustafson, HR, Hashim, K, Hong, S, Jones, LW, Kim, SB, Longo, MJ, Mann, J, Marcin, MR, Neal, HA, Nitz, D, Roe, BP, Snow, G, Thun, R, Wu, D, Zhang, S, Border, P, Courant, H, Gray, R, Heller, K, Kubota, Y, Marshak, M, Peterson, E, Poling, R, Ruddick, K, Kulchitsky, JA, Moroz, LG, Moore, D, Summers, D, Nakamura, T, Nakamura, M, Niwa, K, Miyano, K, Miyata, H, Bishop, J, Biswas, N, Cason, N, Godfrey, J, Kenney, VP, Piekarz, J, Ruchti, R, Shephard, W, Alley, G, Alsmiller, RG, Alsmiller, FS, Fu, CY, Glover, CW, Mahall, J, Ryan, T, Vandergriff, D, Byslma, B, Durkin, LS, Ling, TY, Park, SK, Romanowski, TA, Tamura, N, Okusawa, T, Takahashi, T, Teramoto, Y, Yoshida, T, Nagashima, Y, Sugimoto, S, Bibby, J, Cashmore, R, Harnew, N, Nickerson, R, Williams, W, Gladney, L, Hollebeek, RJ, Newcomer, M, Van Berg, R, Williams, HH, Armstrong, TA, Hartman, KW, Hasan, A, Heppelmann, SF, Lewis, RA, Minor, ED, Oh, BY, Smith, GA, Toothacker, WS, Whitmore, J, Zhang, Y, Amendolia, R, Bedeschi, F, Bellettini, G, Galeotti, S, Grassman, H, Mangano, ML, Menzione, A, Pauletta, G, Passuello, D, Punzi, G, Ristori, L, Engels, EE, Humanic, T, Shepard, PF, Barnes, VE, Garfinkel, AF, Koltick, DS, Laasanen, AT, McIlwain, R, Miller, DH, Shibata, E, Shipsey, IP, Adams, D, Ahmad, S, Bonner, B, Corcoran, M, Miettinen, H, Mutchler, G, Roberts, J, Skeens, J, Bodek, A, Kanda, S, Lobkowicz, F, Sill, A, Slattery, P, Thorndike, EH, Appolinari, G, Giokaris, N, Goulianos, K, Melese, P, Rusack, R, Vacchi, A, White, S, Devlin, T, Watts, T, Edwards, M, Gee, N, Grayer, G, Bonamy, P, Ernwein, J, Hubbard, R, Le Du, P, Pansart, J -P, Rondeaux, F, Murakami, A, Kobayashi, S, Masuda, K, Tsenov, RV, Iordanov, AB, Bintinger, D, Coupal, D, Fry, A, Johnstad, H, Siegrist, J, Turcotte, M, Aliev, Sh, Kan, S, Khaneles, A, Pak, A, Surin, E, Yuldashev, B, Alimov, M, Gulamov, K, Kaprior, V, Myalkovsky, V, Turdaliev, K, Yuldashev, A, Amaglobeli, NS, Chiladze, BG, Hubua, DI, Salukvadze, RG, Grunhaus, J, Heifetz, R, Levy, A, Barasch, E, Bowcock, TJV, Huson, FR, McIntyre, PM, White, J T, Cantrell, CD, Chaney, RC, Fenyves, EJ, Hammack, H, Orgeron, J, Lowery, WB, Johnson, NP, Higuchi, M, Hoshi, Y, Abe, K, Hasegawa, K, Yuta, H, Kato, S, Nishikawa, K, Homma, S, Miyachi, T, Kaneyuki, K, Tanimori, T, Watanabe, Y, Chiba, M, Hamatsu, R, Hirose, T, Emura, T, Takahashi, K, Bailey, DC, Luste, GJ, Martin, JF, Orr, RS, Prentice, JD, Sinervo, P, Yoon, TS, Fujiwara, I, Funayama, Y, Hara, K, Iinuma, T, Kaneko, T, Kim, S, Kondo, K, Miyashita, S, Morita, Y, Nakano, I, Takano, M, Takikawa, K, Yasuoka, K, Asano, Y, Mori, S, Takada, Y, Kafka, T, Mann, WA, Milburn, RH, Napier, A, Sliwa, K, Lu, B, Mo, LW, Nunamaker, TA, Piilonen, LE, Daigo, M, Davisson, RJ, Liang, G, Lubatti, HJ, Wilkes, RJ, Zhao, T, Bellinger, J, Carlsmith, D, Cherwinka, J, Erwin, A, Feyzi, F, Foudas, C, Lackey, J, Loveless, R, Ott, G, Reeder, DD, Smith, W, Wendt, C, Wu, SL, Frisken, WR, Hasell, D, Koniuk, R, Courtney, W, Fisher, S, Elam, A, Poole, E, Caprio, C, Kapcio, P, Buddle, B, Gerace, T, Arens, JF, Jernigan, JG, Atlas, G, Barkan, Ol, Collins, T, Kramer, G, Pfeiffer, C, Wheeler, B, Wolfe, D, Worley, S, Anderson, EJ, Petroff, MD, Brown, J, Dittert, L, McGinley, W, Nunez, A, Riddle, M, Klokow, D, VanderHave, L, Shapiro, SL, Burke, MA, Einolf, C W, Hackworth, DT, Marschik, D, Scherbarth, DW, Swensrud, RL, Toms, JM, SDC Collaboration, Trilling, GH, Berger, EL, Blair, RE, Dawson, JW, Ekenberg, TL, Derrick, M, Fields, TH, Guarino, V, Hagstrom, RT, Hill, NF, Job, P, Kirk, TBW, May, EN, Nasiatka, J, Nodulman, LJ, Price, LE, Proudfoot, J, Spinka, HM, Talaga, RL, Trost, HJ, Underwood, DG, Wagner, RG, Wicklund, AB, Wu, MM, Johns, KA, Cui, Hua-chuan, Gao, Wen-xiu, Huang, De-qiang, Li, Wei-guo, Mao, Hui-shun, Ni, Hui-ling, Qi, Na-ding, Wang, Tai-jie, Yan, Wu-guang, Ye, Ming-han, Zhao, Wei-ren, Zheng, Liu-sheng, Zhou, Yue-hua, Ming, He Yu, Xi, Lai Chu, Tao, Liu Hong, Qiu, Liu Song, Qiao, Lou Bing, Xiang, Yang Ji, De, Yao Shu, Ju, Zhang Re, Behrends, S, Bensinger, JR, Blocker, C, Kesten, P, Kirsch, L, Povinec, P, Strmen, P, Foster, B, Heath, GP, Cutts, D, Gao, GS, Partridge, R, Alexa, A, Horoi, M, Pantea, D, Pentia, M, Petrascu, C, Weinstein, AJ, Gunion, JF, Pellett, D, Mani, S, Lankford, A, Arisaka, K, Bengtsson, HU, Buchanan, C, Chrisman, D, Cline, D, Hauser, J, Muller, T, Park, J, Roberts, D, Slater, W, Ellison, J, Wimpenny, SJ, Sivertz, M, Thomas, D, DeWitt, J, Dorfan, D, Heusch, C, Hubbard, B, Hutchinson, D, Litke, AL, Lockman, WS, Nilsson, W, O'Shaughnessy, K, Pitzl, D, Rowe, W, Sadrozinski, H, Seiden, A, Spencer, E, Armitage, J, Dixit, MS, Estabrooks, P, Godfrey, S, Losty, M, Mes, H, Oakham, G, O'Neille, M, Kawai, H, Campagneri, C, Contreras, M, Eno, S, Frisch, H, Gross-Pilcher, C, Miller, M, Rosenberg, L, Sanders, H, Shochet, M, Sullivan, G, Baranko, GJ, Cheung, HWK, Cumalat, JP, Erdos, E, Ford, WT, Nauenberg, U, Rankin, P, Schultz, G, Smith, JG, Astakhov, VI, Batyunya, BV, Bischoff, A, Budagov, YA, Chuenko, AM, Dokshin, AI, Finger, M, Gerasimov, SB, Golovatyuk, VM, Gotra, Yu N, Gusar, Yu S, Guzik, Z, Khubua, DI, Ilyin, Yu V, Kashigin, SV, Kharzheev, YN, Kolpakov, IF, Kovalenko, AD, Levchanovsky, FV, Lomakin, YF, Malakhov, AI, Matyushevsky, EA, Omelyanenko, AA, Pakhmutov, Yu S, Panebratsev, YA, Puzynin, IV, Semenov, AA, Senner, AE, Shabunov, AV, Sidorov, VT, Sinaev, AN, Sisakian, AN, Smirnov, V, Spassov, T, Tsyganov, EN, Tyapkin, IA, Vasilev, LA, Velev, GV, Vinogradov, VB, Vodopyanov, AS, Vrba, V, Zanevsky, Yu V, Zhuravlev, NI, Zimin, NI, Zinchenko, AI, Goshaw, AT, Oh, SH, Phillips, TJ, Robertson, WJ, Simpkins, JD, Walker, WD, Amatuni, AC, Vartapetian, GA, Areti, VH, Atac, M, Barsotti, E, Bartoszek, L, Baumbaugh, AE, Beretvas, A, Bernstein, R, Binkley, M, Bross, AD, Clark, AG, Cooper, JW, Denby, BH, Denisenko, KG, Denisenko, NL, Droege, T, Eartly, DP, Elias, JE, Fast, RW, Finley, D, Foster, GW, Freeman, J, Gaines, I, Gourlay, SA, Green, DR, Grimson, J, Grozis, C, Hahn, SR, Harris, RM, Hoff, J, Huth, J, Hylen, J, Kephart, RD, Kilmer, J, Krebs, HJ, Kuzminski, J, Lee, A, Limon, PJ, Martin, PS, Mukerjee, A, Nash, T, Newman-Holmes, C, Para, A, Patrick, J, Plunkett, R, Schmidt, EE, Segler, SL, Stanek, RP, Srefanik, A, Stredde, HJ, Tkaczyk, S, Vidal, R, Wagner, RL, Wands, RH, Yarema, R, Yeh, GP, Yoh, J, Zimmerman, T, Field, R, Harmon, J, Walker, J, Corden, M, Hagopian, V, Johnson, K, Wahl, H, Kawaguchi, M, Yoshida, H, Dvornik, AM, Maksimenko, NB, Brandenburg, G, Feldman, G, Franklin, M, Geer, S, Konigsberg, J, Oliver, J, Sadowski, E, Schlabach, P, Wilson, R, Kenney, C, Parker, S, Chiba, Y, Ohsugi, T, Asai, M, Shioden, M, Goldberg, H, Margulies, S, Solomon, J, Downing, R, Errede, S, Gautier, A, Haney, M, Holloway, L, Karliner, I, Liss, A, O'Halloran, T, Thaler, J, Sheldon, P, Simaitis, V, Wiss, J, Blockus, D, Brabson, B, Dzierba, A, Foster, R, Hanson, G, Lou, X, Luehring, F, Martin, B, Ogren, H, Rust, D, Wente, E, Hauptman, J, Bagger, JA, Barnett, BA, Blumenfeld, BJ, Fisher, PH, Matthews, JAJ, Abe, F, Amako, K, Arai, Y, Doi, Y, Fujii, H, Fukui, Y, Haruyama, T, Ikeda, H, Inaba, S, Inagaki, T, Iwasaki, H, Kabe, S, Kanematsu, N, Kanzaki, J, Kondo, T, Maki, A, Manabe, A, Mishina, M, Noumachi, M, Odaka, S, Ogawa, K, Ohska, TK, Sakai, Y, Sakamoto, H, Sasaki, O, Shinkawa, T, Takaiwa, Y, Terada, S, Tsuboyama, T, Tsukada, K, Ujiie, N, Unno, Y, Watase, Y, Yamamoto, A, Yasu, Y, Krivan, F, Seman, M, Spalek, J, Kikuchi, R, Miyake, K, Abrams, GS, Barbaro-Galtieri, A, Barnett, RM, Cahn, RN, Corradi, CA, Eberhard, PH, Einsweiler, K, Edwards, WR, Ely, R, Gilchriese, MGD, Groom, DE, Haber, C, Hearty, C, Hinchliffe, I, Hoff, M, Jared, R, Kadel, RW, Kadyk, JA, Kleinfelder, S, Levi, ME, Lim, A, Loken, SC, Madden, N, Minamihara, YY, Milgrome, O, Millaud, J, Moore, TL, Nygren, DR, Palounek, APT, Pope, WL, Pripstein, M, Rasson, J, Shapiro, M, Shuman, D, Spieler, HG, Stone, R, Strovink, M, Thur, W, Weidenbach, RC, Wenzel, WA, Ziock, H, Bailey, J, Beck, GA, Dainton, JB, Gabathuler, E, Maxfield, SJ, Smith, G, Baden, AR, Ball, AH, Chang, CY, Fong, DG, Goodman, JA, Hadley, NJ, Jawahery, A, Kellogg, RG, Kunori, S, Skuja, A, Zorn, GT, Ragan, K, Stairs, DG, Amidei, D, Ball, RC, Campbell, M, Chapman, J, De, K, Derwent, P, Gustafson, HR, Hashim, K, Hong, S, Jones, LW, Kim, SB, Longo, MJ, Mann, J, Marcin, MR, Neal, HA, Nitz, D, Roe, BP, Snow, G, Thun, R, Wu, D, Zhang, S, Border, P, Courant, H, Gray, R, Heller, K, Kubota, Y, Marshak, M, Peterson, E, Poling, R, Ruddick, K, Kulchitsky, JA, Moroz, LG, Moore, D, Summers, D, Nakamura, T, Nakamura, M, Niwa, K, Miyano, K, Miyata, H, Bishop, J, Biswas, N, Cason, N, Godfrey, J, Kenney, VP, Piekarz, J, Ruchti, R, Shephard, W, Alley, G, Alsmiller, RG, Alsmiller, FS, Fu, CY, Glover, CW, Mahall, J, Ryan, T, Vandergriff, D, Byslma, B, Durkin, LS, Ling, TY, Park, SK, Romanowski, TA, Tamura, N, Okusawa, T, Takahashi, T, Teramoto, Y, Yoshida, T, Nagashima, Y, Sugimoto, S, Bibby, J, Cashmore, R, Harnew, N, Nickerson, R, Williams, W, Gladney, L, Hollebeek, RJ, Newcomer, M, Van Berg, R, Williams, HH, Armstrong, TA, Hartman, KW, Hasan, A, Heppelmann, SF, Lewis, RA, Minor, ED, Oh, BY, Smith, GA, Toothacker, WS, Whitmore, J, Zhang, Y, Amendolia, R, Bedeschi, F, Bellettini, G, Galeotti, S, Grassman, H, Mangano, ML, Menzione, A, Pauletta, G, Passuello, D, Punzi, G, Ristori, L, Engels, EE, Humanic, T, Shepard, PF, Barnes, VE, Garfinkel, AF, Koltick, DS, Laasanen, AT, McIlwain, R, Miller, DH, Shibata, E, Shipsey, IP, Adams, D, Ahmad, S, Bonner, B, Corcoran, M, Miettinen, H, Mutchler, G, Roberts, J, Skeens, J, Bodek, A, Kanda, S, Lobkowicz, F, Sill, A, Slattery, P, Thorndike, EH, Appolinari, G, Giokaris, N, Goulianos, K, Melese, P, Rusack, R, Vacchi, A, White, S, Devlin, T, Watts, T, Edwards, M, Gee, N, Grayer, G, Bonamy, P, Ernwein, J, Hubbard, R, Le Du, P, Pansart, J -P, Rondeaux, F, Murakami, A, Kobayashi, S, Masuda, K, Tsenov, RV, Iordanov, AB, Bintinger, D, Coupal, D, Fry, A, Johnstad, H, Siegrist, J, Turcotte, M, Aliev, Sh, Kan, S, Khaneles, A, Pak, A, Surin, E, Yuldashev, B, Alimov, M, Gulamov, K, Kaprior, V, Myalkovsky, V, Turdaliev, K, Yuldashev, A, Amaglobeli, NS, Chiladze, BG, Hubua, DI, Salukvadze, RG, Grunhaus, J, Heifetz, R, Levy, A, Barasch, E, Bowcock, TJV, Huson, FR, McIntyre, PM, White, J T, Cantrell, CD, Chaney, RC, Fenyves, EJ, Hammack, H, Orgeron, J, Lowery, WB, Johnson, NP, Higuchi, M, Hoshi, Y, Abe, K, Hasegawa, K, Yuta, H, Kato, S, Nishikawa, K, Homma, S, Miyachi, T, Kaneyuki, K, Tanimori, T, Watanabe, Y, Chiba, M, Hamatsu, R, Hirose, T, Emura, T, Takahashi, K, Bailey, DC, Luste, GJ, Martin, JF, Orr, RS, Prentice, JD, Sinervo, P, Yoon, TS, Fujiwara, I, Funayama, Y, Hara, K, Iinuma, T, Kaneko, T, Kim, S, Kondo, K, Miyashita, S, Morita, Y, Nakano, I, Takano, M, Takikawa, K, Yasuoka, K, Asano, Y, Mori, S, Takada, Y, Kafka, T, Mann, WA, Milburn, RH, Napier, A, Sliwa, K, Lu, B, Mo, LW, Nunamaker, TA, Piilonen, LE, Daigo, M, Davisson, RJ, Liang, G, Lubatti, HJ, Wilkes, RJ, Zhao, T, Bellinger, J, Carlsmith, D, Cherwinka, J, Erwin, A, Feyzi, F, Foudas, C, Lackey, J, Loveless, R, Ott, G, Reeder, DD, Smith, W, Wendt, C, Wu, SL, Frisken, WR, Hasell, D, Koniuk, R, Courtney, W, Fisher, S, Elam, A, Poole, E, Caprio, C, Kapcio, P, Buddle, B, Gerace, T, Arens, JF, Jernigan, JG, Atlas, G, Barkan, Ol, Collins, T, Kramer, G, Pfeiffer, C, Wheeler, B, Wolfe, D, Worley, S, Anderson, EJ, Petroff, MD, Brown, J, Dittert, L, McGinley, W, Nunez, A, Riddle, M, Klokow, D, VanderHave, L, Shapiro, SL, Burke, MA, Einolf, C W, Hackworth, DT, Marschik, D, Scherbarth, DW, Swensrud, RL, and Toms, JM

27. Expression of interest by the Solenoidal Detector Collaboration to construct and operate a detector at the Superconducting Super Collider

Author: SDC Collaboration, Trilling, GH, Berger, EL, Blair, RE, Dawson, JW, Derrick, M, Fields, TH, Hagstrom, RT, Hill, NF, Job, P, Kirk, TB, May, EN, Nodulman, LJ, Price, LE, Proudfoot, J, Spinka, HM, Talaga, RL, Trost, HJ, Underwood, DG, Wagner, RG, Wicklund, A B, Johns, KA, Behrends, S, Bensinger, JR, Blocker, C, Kesten, P, Kirsch, L, Povinec, P, Strmen, P, Foster, B, Heath, GP, Cutts, D, Partridge, R, Pellett, D, Arisaka, K, Chrisman, D, Cline, D, Park, J, Roberts, D, Slater, W, Yamamoto, H, Ellison, J, Wimpenny, SJ, Sivertz, M, Thomas, D, Dorfan, D, Heusch, C, Hubbard, B, Litke, AL, Lockman, WS, Pitzl, D, Sadrozinski, H, Seiden, A, Kawai, H, Campagneri, C, Eno, S, Frisch, H, Gross-Pilcher, C, Miller, M, Rosenberg, L, Shochet, M, Sullivan, G, Baranko, GJ, Carr, J, Cheung, HWK, Cumalat, JP, Ford, WT, Nauenberg, U, Rankin, P, Smith, JG, Astakhov, VI, Batyunya, BV, Bischoff, A, Budagov, YA, Denisenko, KG, Denisenko, NL, Gerasimov, SB, Golovatyuk, VM, Guzik, Z, Khubua, DI, Kadyrov, R, Kharzjeev, YN, Kolpakov, IF, Kovalenko, AD, Levchanovsky, FV, Lomakin, YF, Malakhov, AI, Omelyanenko, AA, Panebratsev, YA, Puzynin, IV, Semenov, AA, Senner, AE, Sidorov, VT, Sinaev, AN, Sisakian, AN, Smirnov, V, Spassof, T, Tsyganov, EN, Tyapkin, IA, Velev, GV, Vinogradov, VB, Vodopyanov, AS, Brba, V, Zanevsky, Yu V, Zhuravlev, NI, Zimin, NI, Zinchenko, AI, Fortney, LR, Goshaw, AT, Kowald, W, Oh, SH, Robertson, WJ, Walker, WD, Amatuni, AC, Vartapetian, GA, Amidei, D, Atac, M, Baumbaugh, AE, Beretvas, A, Bernstein, R, Binkley, M, Bross, AD, Clark, AG, Cooper, JW, Eartly, DP, Elias, JE, Fast, R W, Finley, D, Foster, G W, Freeman, J, Gaines, I, Gourlay, SA, Green, DR, Hahn, SR, Harris, RM, Hauser, J, Huth, J, Kephart, RD, Kuzminski, J, Martin, PS, Mishina, M, Mukerjee, A, Nash, T, Newman-Holmes, C, Para, A, Patrick, J, Plunkett, R, Schmidt, EE, Segler, SL, Tkaczyk, S, Vidal, R, Wagner, RL, Yeh, GP, Yoh, J, Field, R, Harmon, J, Walker, J, Corden, M, Hagopian, V, Johnson, K, Wahl, H, Kawaguchi, M, Yoshida, H, Dvornik, AM, Maksimenko, NB, Brandenburg, G, Feldman, G, Franklin, M, Geer, S, Konigsberg, J, Oliver, J, Phillips, T, Wilson, R, Kenney, C, Parker, S, Chiba, Y, Ohsugi, T, Asai, M, Shioden, M, Goldberg, H, Margulies, S, Solomon, J, Downing, R, Errede, S, Gautier, A, Haney, M, Holloway, L, Karliner, I, Liss, A, O'Halloran, T, Thaler, J, Sheldon, P, Simaitis, V, Wiss, J, Blockus, D, Brabson, B, Dzierba, A, Hanson, G, Lou, X, Ogren, H, Rust, D, Hauptman, J, Bagger, JA, Barnett, BA, Blumenfeld, BJ, Fisher, PH, Matthews, JAJ, Abe, F, Amako, K, Arai, Y, Doi, Y, Fujii, H, Fukui, Y, Haruyama, T, Ikeda, H, Ikeda, M, Inaba, S, Inagaki, T, Iwasaki, H, Kabe, S, Kanzaki, J, Kim, SK, Kondo, T, Maki, A, Manabe, A, Noumachi, M, Odaka, S, Ogawa, K, Sakai, Y, Sakamoto, H, Shinkawa, T, Takaiwa, Y, Terada, S, Tsuboyama, T, Tsukada, K, Ujiie, N, Unno, Y, Watase, Y, Yamamoto, A, Yasu, Y, Krivan, F, Seman, M, Spalek, J, Kikuchi, R, Miyake, K, Abrams, GS, Barbaro-Galtieri, A, Barnett, RM, Cahn, RN, Eberhard, PH, Einsweiler, K, Ely, R, Gilchriese, MGD, Groom, DE, Haber, C, Hearty, C, Hinchliffe, I, Kadel, RW, Kadyk, JA, Levi, ME, Limon, PJ, Loken, SC, Nygren, DR, Palounek, APT, Pripstein, M, Shapiro, M, Siegrist, JL, Spieler, HG, Strovink, M, Wang, EM, Wenzel, WA, Bailey, J, Beck, GA, Dainton, JB, Gabathuler, E, Maxfield, SJ, Baden, AR, Ball, AH, Chang, CY, Fong, DG, Goodman, JA, Hadley, NJ, Jawahery, A, Kellogg, RG, Kunori, S, Skuja, A, Zorn, GT, Ball, RC, Campbell, M, Chapman, J, Gustafson, HR, Hong, S, Jones, LW, Longo, MJ, Marcin, MR, Neal, HA, Nitz, D, Roe, BP, Snow, G, Thun, R, Border, P, Courant, H, Heller, K, Kubota, Y, Marshak, M, Peterson, E, Poling, R, Ruddick, K, Kulchitsky, JA, Moroz, LG, Moore, D, Summers, D, Nakamura, T, Nakamura, M, Niwa, K, Miyano, K, Miyata, H, Bishop, J, Biswas, N, Cason, N, Godfrey, J, Kenney, VP, Piekarz, J, Ruchti, R, Shephard, W, Alley, G, Alsmiller, RG, Alsmiller, FS, Fu, CY, Glover, CW, Vandergriff, D, Byslma, B, Durkin, LS, Ling, TY, Park, SK, Romanowski, TA, Tamura, N, Okusawa, T, Takahashi, T, Teramoto, Y, Yoshida, T, Nagashima, Y, Sugimoto, S, Cashmore, R, Harnew, N, Nickerson, R, Weidberg, A, Williams, W, Gladney, L, Hollebeek, RJ, Newcomer, M, Ragan, KJ, Sinervo, PK, Williams, HH, Armstrong, TA, Hartman, KW, Hasan, A, Heppelmann, SF, Lewis, RA, Minor, ED, Oh, BY, Smith, GA, Toothacker, WS, Whitmore, J, Amendolia, R, Bedeschi, F, Bellettini, G, Galeotti, S, Grassman, H, Mangano, ML, Menzione, A, Pauletta, G, Passuello, D, Punzi, G, Ristori, L, Engels, EE, Humanic, T, Mani, S, Shepard, PF, Barnes, VE, Garfinkel, AF, Koltick, DS, Laasanen, AT, McIlwain, R, Miller, DH, Shibata, E, Shipsey, IP, Adams, D, Ahmad, S, Bonner, B, Corcoran, M, Miettinen, H, Mutchler, G, Roberts, J, Skeens, J, Bodek, A, Lobkowicz, F, Sill, A, Slattery, P, Thorndike, EH, Giodaris, N, Goulianos, K, Melese, P, Rusack, R, White, S, Devlin, T, Watts, T, Gee, N, Harvey, JA, Murakami, A, Kobayashi, S, Masuda, K, Tsenov, RV, Iordanov, AB, Lankford, A, Bintinger, D, Johnstad, H, Aliev, Sh, Alimov, M, Gulamov, K, Kan, S, Kaprior, V, Khaneles, A, Myalkovsky, V, Pak, A, Surlin, E, Turdaliev, K, Yuldashev, A, Yuldashev, B, Amaglobeli, NS, Chiladze, BG, Hubua, DI, Salukvadze, RG, McIntyre, PM, Bowcock, TJV, Huson, FR, White, J T, Chaney, RC, Fenyves, EJ, Hammack, H, Orgeron, J, Lowery, WB, Johnson, NP, Higuchi, M, Hoshi, Y, Abe, K, Hasegawa, K, Yuta, H, Kato, S, Nishikawa, K, Homma, S, Miyachi, T, Watanabe, Y, Tanimori, T, Chiba, M, Hamatsu, R, Hirose, T, Kitamura, S, Emura, T, Takahashi, K, Funayama, Y, Hara, K, Kanda, S, Kaneko, T, Kim, S, Kondo, K, Mimashi, T, Miyashita, S, Morita, Y, Nakano, I, Sakurabata, H, Takikawa, K, Yasuoka, K, Asano, Y, Mori, S, Takada, Y, Kafka, T, Mann, WA, Milburn, RH, Napier, A, Sliwa, K, Lu, B, Mo, LW, Piilonen, LE, Daigo, M, Davisson, RJ, Liang, G, Lubatti, HJ, Wilkes, RJ, Zhao, T, Bellinger, J, Carlsmith, D, Erwin, A, Foudas, C, Handler, R, Loveless, R, Ott, G, Reeder, DD, Smith, W, Wendt, C, Wu, SL, SDC Collaboration, Trilling, GH, Berger, EL, Blair, RE, Dawson, JW, Derrick, M, Fields, TH, Hagstrom, RT, Hill, NF, Job, P, Kirk, TB, May, EN, Nodulman, LJ, Price, LE, Proudfoot, J, Spinka, HM, Talaga, RL, Trost, HJ, Underwood, DG, Wagner, RG, Wicklund, A B, Johns, KA, Behrends, S, Bensinger, JR, Blocker, C, Kesten, P, Kirsch, L, Povinec, P, Strmen, P, Foster, B, Heath, GP, Cutts, D, Partridge, R, Pellett, D, Arisaka, K, Chrisman, D, Cline, D, Park, J, Roberts, D, Slater, W, Yamamoto, H, Ellison, J, Wimpenny, SJ, Sivertz, M, Thomas, D, Dorfan, D, Heusch, C, Hubbard, B, Litke, AL, Lockman, WS, Pitzl, D, Sadrozinski, H, Seiden, A, Kawai, H, Campagneri, C, Eno, S, Frisch, H, Gross-Pilcher, C, Miller, M, Rosenberg, L, Shochet, M, Sullivan, G, Baranko, GJ, Carr, J, Cheung, HWK, Cumalat, JP, Ford, WT, Nauenberg, U, Rankin, P, Smith, JG, Astakhov, VI, Batyunya, BV, Bischoff, A, Budagov, YA, Denisenko, KG, Denisenko, NL, Gerasimov, SB, Golovatyuk, VM, Guzik, Z, Khubua, DI, Kadyrov, R, Kharzjeev, YN, Kolpakov, IF, Kovalenko, AD, Levchanovsky, FV, Lomakin, YF, Malakhov, AI, Omelyanenko, AA, Panebratsev, YA, Puzynin, IV, Semenov, AA, Senner, AE, Sidorov, VT, Sinaev, AN, Sisakian, AN, Smirnov, V, Spassof, T, Tsyganov, EN, Tyapkin, IA, Velev, GV, Vinogradov, VB, Vodopyanov, AS, Brba, V, Zanevsky, Yu V, Zhuravlev, NI, Zimin, NI, Zinchenko, AI, Fortney, LR, Goshaw, AT, Kowald, W, Oh, SH, Robertson, WJ, Walker, WD, Amatuni, AC, Vartapetian, GA, Amidei, D, Atac, M, Baumbaugh, AE, Beretvas, A, Bernstein, R, Binkley, M, Bross, AD, Clark, AG, Cooper, JW, Eartly, DP, Elias, JE, Fast, R W, Finley, D, Foster, G W, Freeman, J, Gaines, I, Gourlay, SA, Green, DR, Hahn, SR, Harris, RM, Hauser, J, Huth, J, Kephart, RD, Kuzminski, J, Martin, PS, Mishina, M, Mukerjee, A, Nash, T, Newman-Holmes, C, Para, A, Patrick, J, Plunkett, R, Schmidt, EE, Segler, SL, Tkaczyk, S, Vidal, R, Wagner, RL, Yeh, GP, Yoh, J, Field, R, Harmon, J, Walker, J, Corden, M, Hagopian, V, Johnson, K, Wahl, H, Kawaguchi, M, Yoshida, H, Dvornik, AM, Maksimenko, NB, Brandenburg, G, Feldman, G, Franklin, M, Geer, S, Konigsberg, J, Oliver, J, Phillips, T, Wilson, R, Kenney, C, Parker, S, Chiba, Y, Ohsugi, T, Asai, M, Shioden, M, Goldberg, H, Margulies, S, Solomon, J, Downing, R, Errede, S, Gautier, A, Haney, M, Holloway, L, Karliner, I, Liss, A, O'Halloran, T, Thaler, J, Sheldon, P, Simaitis, V, Wiss, J, Blockus, D, Brabson, B, Dzierba, A, Hanson, G, Lou, X, Ogren, H, Rust, D, Hauptman, J, Bagger, JA, Barnett, BA, Blumenfeld, BJ, Fisher, PH, Matthews, JAJ, Abe, F, Amako, K, Arai, Y, Doi, Y, Fujii, H, Fukui, Y, Haruyama, T, Ikeda, H, Ikeda, M, Inaba, S, Inagaki, T, Iwasaki, H, Kabe, S, Kanzaki, J, Kim, SK, Kondo, T, Maki, A, Manabe, A, Noumachi, M, Odaka, S, Ogawa, K, Sakai, Y, Sakamoto, H, Shinkawa, T, Takaiwa, Y, Terada, S, Tsuboyama, T, Tsukada, K, Ujiie, N, Unno, Y, Watase, Y, Yamamoto, A, Yasu, Y, Krivan, F, Seman, M, Spalek, J, Kikuchi, R, Miyake, K, Abrams, GS, Barbaro-Galtieri, A, Barnett, RM, Cahn, RN, Eberhard, PH, Einsweiler, K, Ely, R, Gilchriese, MGD, Groom, DE, Haber, C, Hearty, C, Hinchliffe, I, Kadel, RW, Kadyk, JA, Levi, ME, Limon, PJ, Loken, SC, Nygren, DR, Palounek, APT, Pripstein, M, Shapiro, M, Siegrist, JL, Spieler, HG, Strovink, M, Wang, EM, Wenzel, WA, Bailey, J, Beck, GA, Dainton, JB, Gabathuler, E, Maxfield, SJ, Baden, AR, Ball, AH, Chang, CY, Fong, DG, Goodman, JA, Hadley, NJ, Jawahery, A, Kellogg, RG, Kunori, S, Skuja, A, Zorn, GT, Ball, RC, Campbell, M, Chapman, J, Gustafson, HR, Hong, S, Jones, LW, Longo, MJ, Marcin, MR, Neal, HA, Nitz, D, Roe, BP, Snow, G, Thun, R, Border, P, Courant, H, Heller, K, Kubota, Y, Marshak, M, Peterson, E, Poling, R, Ruddick, K, Kulchitsky, JA, Moroz, LG, Moore, D, Summers, D, Nakamura, T, Nakamura, M, Niwa, K, Miyano, K, Miyata, H, Bishop, J, Biswas, N, Cason, N, Godfrey, J, Kenney, VP, Piekarz, J, Ruchti, R, Shephard, W, Alley, G, Alsmiller, RG, Alsmiller, FS, Fu, CY, Glover, CW, Vandergriff, D, Byslma, B, Durkin, LS, Ling, TY, Park, SK, Romanowski, TA, Tamura, N, Okusawa, T, Takahashi, T, Teramoto, Y, Yoshida, T, Nagashima, Y, Sugimoto, S, Cashmore, R, Harnew, N, Nickerson, R, Weidberg, A, Williams, W, Gladney, L, Hollebeek, RJ, Newcomer, M, Ragan, KJ, Sinervo, PK, Williams, HH, Armstrong, TA, Hartman, KW, Hasan, A, Heppelmann, SF, Lewis, RA, Minor, ED, Oh, BY, Smith, GA, Toothacker, WS, Whitmore, J, Amendolia, R, Bedeschi, F, Bellettini, G, Galeotti, S, Grassman, H, Mangano, ML, Menzione, A, Pauletta, G, Passuello, D, Punzi, G, Ristori, L, Engels, EE, Humanic, T, Mani, S, Shepard, PF, Barnes, VE, Garfinkel, AF, Koltick, DS, Laasanen, AT, McIlwain, R, Miller, DH, Shibata, E, Shipsey, IP, Adams, D, Ahmad, S, Bonner, B, Corcoran, M, Miettinen, H, Mutchler, G, Roberts, J, Skeens, J, Bodek, A, Lobkowicz, F, Sill, A, Slattery, P, Thorndike, EH, Giodaris, N, Goulianos, K, Melese, P, Rusack, R, White, S, Devlin, T, Watts, T, Gee, N, Harvey, JA, Murakami, A, Kobayashi, S, Masuda, K, Tsenov, RV, Iordanov, AB, Lankford, A, Bintinger, D, Johnstad, H, Aliev, Sh, Alimov, M, Gulamov, K, Kan, S, Kaprior, V, Khaneles, A, Myalkovsky, V, Pak, A, Surlin, E, Turdaliev, K, Yuldashev, A, Yuldashev, B, Amaglobeli, NS, Chiladze, BG, Hubua, DI, Salukvadze, RG, McIntyre, PM, Bowcock, TJV, Huson, FR, White, J T, Chaney, RC, Fenyves, EJ, Hammack, H, Orgeron, J, Lowery, WB, Johnson, NP, Higuchi, M, Hoshi, Y, Abe, K, Hasegawa, K, Yuta, H, Kato, S, Nishikawa, K, Homma, S, Miyachi, T, Watanabe, Y, Tanimori, T, Chiba, M, Hamatsu, R, Hirose, T, Kitamura, S, Emura, T, Takahashi, K, Funayama, Y, Hara, K, Kanda, S, Kaneko, T, Kim, S, Kondo, K, Mimashi, T, Miyashita, S, Morita, Y, Nakano, I, Sakurabata, H, Takikawa, K, Yasuoka, K, Asano, Y, Mori, S, Takada, Y, Kafka, T, Mann, WA, Milburn, RH, Napier, A, Sliwa, K, Lu, B, Mo, LW, Piilonen, LE, Daigo, M, Davisson, RJ, Liang, G, Lubatti, HJ, Wilkes, RJ, Zhao, T, Bellinger, J, Carlsmith, D, Erwin, A, Foudas, C, Handler, R, Loveless, R, Ott, G, Reeder, DD, Smith, W, Wendt, C, and Wu, SL

28. A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies.

Author: McDonald M, Bayliss M, Benson BA, Foley RJ, Ruel J, Sullivan P, Veilleux S, Aird KA, Ashby ML, Bautz M, Bazin G, Bleem LE, Brodwin M, Carlstrom JE, Chang CL, Cho HM, Clocchiatti A, Crawford TM, Crites AT, de Haan T, Desai S, Dobbs MA, Dudley JP, Egami E, Forman WR, Garmire GP, George EM, Gladders MD, Gonzalez AH, Halverson NW, Harrington NL, High FW, Holder GP, Holzapfel WL, Hoover S, Hrubes JD, Jones C, Joy M, Keisler R, Knox L, Lee AT, Leitch EM, Liu J, Lueker M, Luong-Van D, Mantz A, Marrone DP, McMahon JJ, Mehl J, Meyer SS, Miller ED, Mocanu L, Mohr JJ, Montroy TE, Murray SS, Natoli T, Padin S, Plagge T, Pryke C, Rawle TD, Reichardt CL, Rest A, Rex M, Ruhl JE, Saliwanchik BR, Saro A, Sayre JT, Schaffer KK, Shaw L, Shirokoff E, Simcoe R, Song J, Spieler HG, Stalder B, Staniszewski Z, Stark AA, Story K, Stubbs CW, Suhada R, van Engelen A, Vanderlinde K, Vieira JD, Vikhlinin A, Williamson R, Zahn O, and Zenteno A
Abstract: In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the cluster's lifetime, leading to continuous 'cooling flows' of gas sinking towards the cluster centre, yet no such cooling flow has been observed. The low observed star-formation rates and cool gas masses for these 'cool-core' clusters suggest that much of the cooling must be offset by feedback to prevent the formation of a runaway cooling flow. Here we report X-ray, optical and infrared observations of the galaxy cluster SPT-CLJ2344-4243 (ref. 11) at redshift z = 0.596. These observations reveal an exceptionally luminous (8.2 × 10(45) erg s(-1)) galaxy cluster that hosts an extremely strong cooling flow (around 3,820 solar masses a year). Further, the central galaxy in this cluster appears to be experiencing a massive starburst (formation of around 740 solar masses a year), which suggests that the feedback source responsible for preventing runaway cooling in nearby cool-core clusters may not yet be fully established in SPT-CLJ2344-4243. This large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.
Published: 2012
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29. Frequency multiplexed superconducting quantum interference device readout of large bolometer arrays for cosmic microwave background measurements.

Author: Dobbs MA, Lueker M, Aird KA, Bender AN, Benson BA, Bleem LE, Carlstrom JE, Chang CL, Cho HM, Clarke J, Crawford TM, Crites AT, Flanigan DI, de Haan T, George EM, Halverson NW, Holzapfel WL, Hrubes JD, Johnson BR, Joseph J, Keisler R, Kennedy J, Kermish Z, Lanting TM, Lee AT, Leitch EM, Luong-Van D, McMahon JJ, Mehl J, Meyer SS, Montroy TE, Padin S, Plagge T, Pryke C, Richards PL, Ruhl JE, Schaffer KK, Schwan D, Shirokoff E, Spieler HG, Staniszewski Z, Stark AA, Vanderlinde K, Vieira JD, Vu C, Westbrook B, and Williamson R
Abstract: A technological milestone for experiments employing transition edge sensor bolometers operating at sub-Kelvin temperature is the deployment of detector arrays with 100s-1000s of bolometers. One key technology for such arrays is readout multiplexing: the ability to read out many sensors simultaneously on the same set of wires. This paper describes a frequency-domain multiplexed readout system which has been developed for and deployed on the APEX-SZ and South Pole Telescope millimeter wavelength receivers. In this system, the detector array is divided into modules of seven detectors, and each bolometer within the module is biased with a unique ∼MHz sinusoidal carrier such that the individual bolometer signals are well separated in frequency space. The currents from all bolometers in a module are summed together and pre-amplified with superconducting quantum interference devices operating at 4 K. Room temperature electronics demodulate the carriers to recover the bolometer signals, which are digitized separately and stored to disk. This readout system contributes little noise relative to the detectors themselves, is remarkably insensitive to unwanted microphonic excitations, and provides a technology pathway to multiplexing larger numbers of sensors.
Published: 2012
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30. South Pole Telescope optics.

Author: Padin S, Staniszewski Z, Keisler R, Joy M, Stark AA, Ade PA, Aird KA, Benson BA, Bleem LE, Carlstrom JE, Chang CL, Crawford TM, Crites AT, Dobbs MA, Halverson NW, Heimsath S, Hills RE, Holzapfel WL, Lawrie C, Lee AT, Leitch EM, Leong J, Lu W, Lueker M, McMahon JJ, Meyer SS, Mohr JJ, Montroy TE, Plagge T, Pryke C, Ruhl JE, Schaffer KK, Shirokoff E, Spieler HG, and Vieira JD
Abstract: The South Pole Telescope is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, millimeter-wave, bolometer array receiver. The telescope has an unusual optical system with a cold stop around the secondary. The design emphasizes low scattering and low background loading. All the optical components except the primary are cold, and the entire beam from prime focus to the detectors is surrounded by cold absorber.
Published: 2008
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31. The fragmentation of 670A MeV neon-20 as a function of depth in water. I. Experiment.

Author: Schimmerling W, Miller J, Wong M, Rapkin M, Howard J, Spieler HG, and Jarret BV
Subjects: Ions, Particle Accelerators, Water, Neon
Abstract: We present the final analysis of an experiment to study the interaction of a beam of 670A MeV neon ions incident on a water column set to different thicknesses. The atomic number Z (and, in some cases, the isotopic mass A) of primary beam particles and of the products of nuclear interactions emerging from the water column close to the central axis of the beam was obtained for nuclei between Be (Z = 4) and Ne (Z = 10) using a time-of-flight telescope to measure the velocity and a set of silicon detectors to measure the energy loss of each particle. The fluence of particles of a given charge was obtained and normalized to the incident beam intensity. Corrections were made for accidental coincidences between multiple particles triggering the TOF telescope and for interactions in the detector. The background due to beam particles interacting in beam line elements upstream of the detector was calculated. Sources of experimental artifacts and background in particle identification experiments designed to characterize heavy ion beams for radiobiological research are summarized, and some of the difficulties inherent in this work are discussed. Complete tables of absolutely normalized fluence spectra as a function of LET are included for reference purposes.
Published: 1989

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1. COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

2. SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY

3. A MEASUREMENT OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND BY GALAXY CLUSTERS USING DATA FROM THE SOUTH POLE TELESCOPE

4. Analysis of Sunyaev-Zel'dovich effect mass-observable relations using South Pole Telescope observations of an X-ray selected sample of low-mass galaxy clusters and groups

5. MEASUREMENT OF GALAXY CLUSTER INTEGRATED COMPTONIZATION AND MASS SCALING RELATIONS WITH THE SOUTH POLE TELESCOPE

6. GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY

7. A MEASUREMENT OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES FROM THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

8. Optical Spectroscopy and Velocity Dispersions of Galaxy Clusters from the SPT-SZ Survey

9. A MEASUREMENT OF THE SECONDARY-CMB AND MILLIMETER-WAVE-FOREGROUND BISPECTRUM USING 800 deg2 OF SOUTH POLE TELESCOPE DATA

10. THE REDSHIFT EVOLUTION OF THE MEAN TEMPERATURE, PRESSURE, AND ENTROPY PROFILES IN 80 SPT-SELECTED GALAXY CLUSTERS

11. Constraints on the CMB temperature evolution using multiband measurements of the Sunyaev-Zel'dovich effect with the South Pole Telescope

12. SPT-CL J2040-4451: AN SZ-SELECTED GALAXY CLUSTER AT z=1.478 WITH SIGNIFICANT ONGOING STAR FORMATION

13. CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg2 SPT-SZ SURVEY

14. SPT-CL J0205-5829: A z=1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY

15. COSMOLOGICAL CONSTRAINTS FROM SUNYAEV-ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg2 OF THE SOUTH POLE TELESCOPE SURVEY

16. GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY

17. IMPROVED CONSTRAINTS ON COSMIC MICROWAVE BACKGROUND SECONDARY ANISOTROPIES FROM THE COMPLETE 2008 SOUTH POLE TELESCOPE DATA

18. X-RAY PROPERTIES OF THE FIRST SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTER SAMPLE FROM THE SOUTH POLE TELESCOPE

19. SOUTH POLE TELESCOPE DETECTIONS OF THE PREVIOUSLY UNCONFIRMED PLANCK EARLY SUNYAEV-ZEL'DOVICH CLUSTERS IN THE SOUTHERN HEMISPHERE

20. A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE

21. OPTICAL REDSHIFT AND RICHNESS ESTIMATES FOR GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS

22. EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD

23. MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE

24. ANGULAR POWER SPECTRA OF THE MILLIMETER-WAVELENGTH BACKGROUND LIGHT FROM DUSTY STAR-FORMING GALAXIES WITH THE SOUTH POLE TELESCOPE

25. GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS

26. Letter of Intent by the Solenoidal Detector Collaboration to construct and operate a detector at the Superconducting Super Collider

27. Expression of interest by the Solenoidal Detector Collaboration to construct and operate a detector at the Superconducting Super Collider

28. A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies.

29. Frequency multiplexed superconducting quantum interference device readout of large bolometer arrays for cosmic microwave background measurements.

30. South Pole Telescope optics.

31. The fragmentation of 670A MeV neon-20 as a function of depth in water. I. Experiment.

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