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634 results on '"GEORGE, E. M."'

201. The Growth of Cool Cores and Evolution of Cooling Properties in a Sample of 83 Galaxy Clusters at 0.3 < z < 1.2 Selected from the SPT-SZ Survey

Author: McDonald, M., Benson, B. A., Vikhlinin, A., Stalder, B., Bleem, L. E., Lin, H. W., Aird, K. A., Ashby, M. L. N., Bautz, M. W., Bayliss, M., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dobbs, M. A., Dudley, J. P., Foley, R. J., Forman, W. R., George, E. M., Gettings, D., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Jones, C., Joy, M., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Miller, E. D., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Nurgaliev, D., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Song, J., Suhada, R., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., Zenteno, A., McDonald, M., Benson, B. A., Vikhlinin, A., Stalder, B., Bleem, L. E., Lin, H. W., Aird, K. A., Ashby, M. L. N., Bautz, M. W., Bayliss, M., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dobbs, M. A., Dudley, J. P., Foley, R. J., Forman, W. R., George, E. M., Gettings, D., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Jones, C., Joy, M., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Miller, E. D., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Nurgaliev, D., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Song, J., Suhada, R., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., and Zenteno, A.
Abstract: We present first results on the cooling properties derived from Chandra X-ray observations of 83 high-redshift (0.3 < z < 1.2) massive galaxy clusters selected by their Sunyaev-Zel'dovich signature in the South Pole Telescope data. We measure each cluster's central cooling time, central entropy, and mass deposition rate, and compare to local cluster samples. We find no significant evolution from z~0 to z~1 in the distribution of these properties, suggesting that cooling in cluster cores is stable over long periods of time. We also find that the average cool core entropy profile in the inner ~100 kpc has not changed dramatically since z ~ 1, implying that feedback must be providing nearly constant energy injection to maintain the observed "entropy floor" at ~10 keV cm^2. While the cooling properties appear roughly constant over long periods of time, we observe strong evolution in the gas density profile, with the normalized central density (rho_0/rho_crit) increasing by an order of magnitude from z ~ 1 to z ~ 0. When using metrics defined by the inner surface brightness profile of clusters, we find an apparent lack of classical, cuspy, cool-core clusters at z > 0.75, consistent with earlier reports for clusters at z > 0.5 using similar definitions. Our measurements indicate that cool cores have been steadily growing over the 8 Gyr spanned by our sample, consistent with a constant, ~150 Msun/yr cooling flow that is unable to cool below entropies of 10 keV cm^2 and, instead, accumulates in the cluster center. We estimate that cool cores began to assemble in these massive systems at z ~ 1, which represents the first constraints on the onset of cooling in galaxy cluster cores. We investigate several potential biases which could conspire to mimic this cool core evolution and are unable to find a bias that has a similar redshift dependence and a substantial amplitude., Comment: 17 pages with 15 figures, plus appendix. Published in ApJ
Published: 2013
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202. Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope

Author: Hanson, D., Hoover, S., Crites, A., Ade, P. A. R., Aird, K. A., Austermann, J. E., Beall, J. A., Bender, A. N., Benson, B. A., Bleem, L. E., Bock, J. J., Carlstrom, J. E., Chang, C. L., Chiang, H. C., Cho, H-M., Conley, A., Crawford, T. M., de Haan, T., Dobbs, M. A., Everett, W., Gallicchio, J., Gao, J., George, E. M., Halverson, N. W., Harrington, N., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E., Li, D., Liang, C., Luong-Van, D., Marsden, G., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., Natoli, T., Nibarger, J. P., Novosad, V., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Schulz, B., Smecher, G., Stark, A. A., Story, K., Tucker, C., Vanderlinde, K., Vieira, J. D., Viero, M. P., Wang, G., Yefremenko, V., Zahn, O., Zemcov, M., Hanson, D., Hoover, S., Crites, A., Ade, P. A. R., Aird, K. A., Austermann, J. E., Beall, J. A., Bender, A. N., Benson, B. A., Bleem, L. E., Bock, J. J., Carlstrom, J. E., Chang, C. L., Chiang, H. C., Cho, H-M., Conley, A., Crawford, T. M., de Haan, T., Dobbs, M. A., Everett, W., Gallicchio, J., Gao, J., George, E. M., Halverson, N. W., Harrington, N., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E., Li, D., Liang, C., Luong-Van, D., Marsden, G., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., Natoli, T., Nibarger, J. P., Novosad, V., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Schulz, B., Smecher, G., Stark, A. A., Story, K., Tucker, C., Vanderlinde, K., Vieira, J. D., Viero, M. P., Wang, G., Yefremenko, V., Zahn, O., and Zemcov, M.
Abstract: Gravitational lensing of the cosmic microwave background generates a curl pattern in the observed polarization. This "B-mode" signal provides a measure of the projected mass distribution over the entire observable Universe and also acts as a contaminant for the measurement of primordial gravity-wave signals. In this Letter we present the first detection of gravitational lensing B modes, using first-season data from the polarization-sensitive receiver on the South Pole Telescope (SPTpol). We construct a template for the lensing B-mode signal by combining E-mode polarization measured by SPTpol with estimates of the lensing potential from a Herschel-SPIRE map of the cosmic infrared background. We compare this template to the B modes measured directly by SPTpol, finding a non-zero correlation at 7.7 sigma significance. The correlation has an amplitude and scale-dependence consistent with theoretical expectations, is robust with respect to analysis choices, and constitutes the first measurement of a powerful cosmological observable., Comment: Two additional null tests, matches version published in PRL
Published: 2013
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203. SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation

Author: Bayliss, M. B., Ashby, M. L. N., Ruel, J., Brodwin, M., Aird, K. A., Bautz, M. W., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., Dobbs, M. A., Dudley, J. P., Foley, R. J., Forman, W. R., George, E. M., Gettings, D., Gladders, M. D., Gonzalez, A. H., de Haan, T., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Jones, C., Joy, M., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., Mawatari, K., McDonald, M., McMahon, J. J., Mehl, J., Meyer, S. S., Miller, E. D., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Rest, A., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Song, J., Stalder, B., Suhada, R., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K., Stubbs, C. W., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., Zenteno, A., Bayliss, M. B., Ashby, M. L. N., Ruel, J., Brodwin, M., Aird, K. A., Bautz, M. W., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., Dobbs, M. A., Dudley, J. P., Foley, R. J., Forman, W. R., George, E. M., Gettings, D., Gladders, M. D., Gonzalez, A. H., de Haan, T., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Jones, C., Joy, M., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., Mawatari, K., McDonald, M., McMahon, J. J., Mehl, J., Meyer, S. S., Miller, E. D., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Rest, A., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Song, J., Stalder, B., Suhada, R., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K., Stubbs, C. W., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., 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., Comment: 14 pages, 8 figures, 4 tables, Accepted to ApJ
Published: 2013
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204. A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing

Author: Geach, J. E., Hickox, R. C., Bleem, L. E., Brodwin, M., Holder, G. P., Aird, K. A., Benson, B. A., Bhattacharya, S., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Hainline, K. N., Halverson, N. W., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Myers, A. D., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., Geach, J. E., Hickox, R. C., Bleem, L. E., Brodwin, M., Holder, G. P., Aird, K. A., Benson, B. A., Bhattacharya, S., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Hainline, K. N., Halverson, N. W., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Myers, A. D., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., and Zahn, O.
Abstract: We measure the cross-power spectrum of the projected mass density as traced by the convergence of the cosmic microwave background lensing field from the South Pole Telescope (SPT) and a sample of Type 1 and 2 (unobscured and obscured) quasars at z~1 selected with the Wide-field Infrared Survey Explorer, over 2500 deg^2. The cross-power spectrum is detected at ~7-sigma, and we measure a linear bias b=1.67+/-0.24, consistent with clustering analyses. Using an independent lensing map, derived from Planck observations, to measure the cross-spectrum, we find excellent agreement with the SPT analysis. The bias of the combined sample of Type 1 and 2 quasars determined in this work is similar to that previously determined for Type 1 quasars alone; we conclude that that obscured and unobscured quasars must trace the matter field in a similar way. This result has implications for our understanding of quasar unification and evolution schemes., Comment: replaced with version accepted for publication in the Astrophysical Journal Letters, ApJ, 776, L41
Published: 2013
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205. A CMB lensing mass map and its correlation with the cosmic infrared background

Author: Holder, G. P., Viero, M. P., Zahn, O., Aird, K. A., Benson, B. A., Bhattacharya, S., Bleem, L. E., Bock, J., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H-M., Conley, A., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Halverson, N. W., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Marsden, G., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Schulz, B., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zemcov, M., Holder, G. P., Viero, M. P., Zahn, O., Aird, K. A., Benson, B. A., Bhattacharya, S., Bleem, L. E., Bock, J., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H-M., Conley, A., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Halverson, N. W., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Marsden, G., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Schulz, B., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., and Zemcov, M.
Abstract: We use a temperature map of the cosmic microwave background (CMB) obtained using the South Pole Telescope at 150 GHz to construct a map of the gravitational convergence to z ~ 1100, revealing the fluctuations in the projected mass density. This map shows individual features that are significant at the ~ 4 sigma level, providing the first image of CMB lensing convergence. We cross-correlate this map with Herschel/SPIRE maps covering 90 square degrees at wavelengths of 500, 350, and 250 microns. We show that these submillimeter-wavelength (submm) maps are strongly correlated with the lensing convergence map, with detection significances in each of the three submm bands ranging from 6.7 to 8.8 sigma. We fit the measurement of the cross power spectrum assuming a simple constant bias model and infer bias factors of b=1.3-1.8, with a statistical uncertainty of 15%, depending on the assumed model for the redshift distribution of the dusty galaxies that are contributing to the Herschel/SPIRE maps., Comment: 5 pages, 3 figures, to be submitted to ApJL
Published: 2013
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206. Dusty starburst galaxies in the early Universe as revealed by gravitational lensing

Author: Vieira, J. D., Marrone, D. P., Chapman, S. C., De Breuck, C., Hezaveh, Y. D., Weiss, A., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Biggs, A. D., Bleem, L. E., Bock, J. J., Bothwell, M., Bradford, C. M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Fomalont, E. B., Fassnacht, C. D., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Hunter, T. R., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Mocanu, L. M., Murphy, E. J., Natoli, T., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Sharon, K., Schaffer, K. K., Shaw, L., Shirokoff, E., Spilker, J. S., Stalder, B., Staniszewski1, Z., Stark, A. A., Story, K., Vanderlinde, K., Welikala, N., Williamson, R., Vieira, J. D., Marrone, D. P., Chapman, S. C., De Breuck, C., Hezaveh, Y. D., Weiss, A., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Biggs, A. D., Bleem, L. E., Bock, J. J., Bothwell, M., Bradford, C. M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Fomalont, E. B., Fassnacht, C. D., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Hunter, T. R., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Mocanu, L. M., Murphy, E. J., Natoli, T., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Sharon, K., Schaffer, K. K., Shaw, L., Shirokoff, E., Spilker, J. S., Stalder, B., Staniszewski1, Z., Stark, A. A., Story, K., Vanderlinde, K., Welikala, N., and Williamson, R.
Abstract: In the past decade, our understanding of galaxy evolution has been revolutionized by the discovery that luminous, dusty, starburst galaxies were 1,000 times more abundant in the early Universe than at present. It has, however, been difficult to measure the complete redshift 2 distribution of these objects, especially at the highest redshifts (z > 4). Here we report a redshift survey at a wavelength of three millimeters, targeting carbon monoxide line emission from the star-forming molecular gas in the direction of extraordinarily bright millimetrewave-selected sources. High-resolution imaging demonstrates that these sources are strongly gravitationally lensed by foreground galaxies. We detect spectral lines in 23 out of 26 sources and multiple lines in 12 of those 23 sources, from which we obtain robust, unambiguous redshifts. At least 10 of the sources are found to lie at z > 4, indicating that the fraction of dusty starburst galaxies at high redshifts is greater than previously thought. Models of lens geometries in the sample indicate that the background objects are ultra-luminous infrared galaxies, powered by extreme bursts of star formation., Comment: Accepted for publication in Nature. Under press embargo till 18:00 GMT on Wednesday March 13th
Published: 2013
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207. A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data

Author: Crawford, T. M., Schaffer, K. K., Bhattacharya, S., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., Crawford, T. M., Schaffer, K. K., Bhattacharya, S., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., 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., Comment: 23 emulateapj pages, 4 figures, revised to match published version. Data products available at http://pole.uchicago.edu/public/data/crawford13
Published: 2013
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208. ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

Author: Weiss, A., De Breuck, C., Marrone, D. P., Vieira, J. D., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bethermin, M., Biggs, A. D., Bleem, L. E., Bock, J. J., Bothwell, M., Bradford, C. M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chapman, S. C., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Downes, T. P., Fassnacht, C. D., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Halverson, N. W., Hezaveh, Y. D., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Husband, K., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Murphy, E. J., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Rosenman, M., Ruel, J., Ruhl, J. E., Schaffer, K. K., Shirokoff, E., Spilker, J. S., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Vanderlinde, K., Welikala, N., Williamson, R., Weiss, A., De Breuck, C., Marrone, D. P., Vieira, J. D., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bethermin, M., Biggs, A. D., Bleem, L. E., Bock, J. J., Bothwell, M., Bradford, C. M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chapman, S. C., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Downes, T. P., Fassnacht, C. D., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Halverson, N. W., Hezaveh, Y. D., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Husband, K., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Murphy, E. J., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Rosenman, M., Ruel, J., Ruhl, J. E., Schaffer, K. K., Shirokoff, E., Spilker, J. S., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Vanderlinde, K., Welikala, N., and Williamson, R.
Abstract: Using the Atacama Large Millimeter/submillimeter Array (ALMA), we have conducted a blind redshift survey in the 3 mm atmospheric transmission window for 26 strongly lensd dusty star-forming galaxies (DSFGs) selected with the South Pole Telescope (SPT). The sources were selected to have S_1.4mm>20 mJy and a dust-like spectrum and, to remove low-z sources, not have bright radio (S_843MHz<6mJy) or far-infrared counterparts (S_100um<1 Jy, S_60um<200mJy). We robustly detect 44 line features in our survey, which we identify as redshifted emission lines of 12CO, 13CO, [CI], H2O, and H2O+. We find one or more spectral features in 23 sources yielding a ~90% detection rate for this survey; in 12 of these sources we detect multiple lines, while in 11 sources we detect only a single line. For the sources with only one detected line, we break the redshift degeneracy with additional spectroscopic observations if available, or infer the most likely line identification based on photometric data. This yields secure redshifts for ~70% of the sample. The three sources with no lines detected are tentatively placed in the redshift desert between 1.7=3.5. This finding is in contrast to the redshift distribution of radio-identified DSFGs, which have a significantly lower mean redshift of =2.3 and for which only 10-15% of the population is expected to be at z>3. We discuss the effect of gravitational lensing on the redshift distribution and compare our measured redshift distribution to that of models in the literature., Comment: Accepted for publication in the Astrophysical Journal
Published: 2013
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209. ALMA Observations of SPT-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies

Author: Hezaveh, Y. D., Marrone, D. P., Fassnacht, C. D., Spilker, J. S., Vieira, J. D., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bleem, L. E., Bothwell, M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chapman, S. C., Crawford, T. M., Crites, A. T., De Breuck, C., de Haan, T., Dobbs, M. A., Fomalont, E. B., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Husband, K., Hunter, T. R., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Mocanu, L. M., Murphy, E. J., Natoli, T., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Sharon, K., Schaffer, K. K., Shaw, L., Shirokoff, E., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Vanderlinde, K., Weiß, A., Welikala, N., Williamson, R., Hezaveh, Y. D., Marrone, D. P., Fassnacht, C. D., Spilker, J. S., Vieira, J. D., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bleem, L. E., Bothwell, M., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chapman, S. C., Crawford, T. M., Crites, A. T., De Breuck, C., de Haan, T., Dobbs, M. A., Fomalont, E. B., George, E. M., Gladders, M. D., Gonzalez, A. H., Greve, T. R., Halverson, N. W., High, F. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Husband, K., Hunter, T. R., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Malkan, M., McIntyre, V., McMahon, J. J., Mehl, J., Menten, K. M., Meyer, S. S., Mocanu, L. M., Murphy, E. J., Natoli, T., Padin, S., Plagge, T., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Sharon, K., Schaffer, K. K., Shaw, L., Shirokoff, E., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Vanderlinde, K., Weiß, A., Welikala, N., and Williamson, R.
Abstract: We present Atacama Large Millimeter/submillimeter Array (ALMA) 860 micrometer imaging of four high-redshift (z=2.8-5.7) dusty sources that were detected using the South Pole Telescope (SPT) at 1.4 mm and are not seen in existing radio to far-infrared catalogs. At 1.5 arcsec resolution, the ALMA data reveal multiple images of each submillimeter source, separated by 1-3 arcsec, consistent with strong lensing by intervening galaxies visible in near-IR imaging of these sources. We describe a gravitational lens modeling procedure that operates on the measured visibilities and incorporates self-calibration-like antenna phase corrections as part of the model optimization, which we use to interpret the source structure. Lens models indicate that SPT0346-52, located at z=5.7, is one of the most luminous and intensely star-forming sources in the universe with a lensing corrected FIR luminosity of 3.7 X 10^13 L_sun and star formation surface density of 4200 M_sun yr^-1 kpc^-2. We find magnification factors of 5 to 22, with lens Einstein radii of 1.1-2.0 arcsec and Einstein enclosed masses of 1.6-7.2x10^11 M_sun. These observations confirm the lensing origin of these objects, allow us to measure the their intrinsic sizes and luminosities, and demonstrate the important role that ALMA will play in the interpretation of lensed submillimeter sources., Comment: Accepted for publication in the Astrophysics Journal
Published: 2013
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210. The HARMONI/ELT spectrographs

Author: Evans, Christopher J., Simard, Luc, Takami, Hideki, Rodrigues, M., Capone, J., Earle, A., Foster, T., Hidalgo, A., Lewis, I., Lynn, J., O'brien, K., Tosh, I., George, E. M., Accardo, M., Alvarez, D., Conzelmann, R., Hopgood, J., Clarke, F., Schnetler, H., Tecza, M., and Thatte, N.
Published: 2018
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211. Short report: Churg Strauss syndrome (allergic granulomatous angiitis) as a cause of central retinal artery occlusion

Author: Johannes L. J. M. Teepen, George E. M. Kienstra, Louis A. K. Bastiaensen, and Willem P. L. Van Boven
Subjects: medicine.medical_specialty, medicine.diagnostic_test, Cyclophosphamide, business.industry, Retinal arterial occlusion, Churg-strauss syndrome, Signs and symptoms, medicine.disease, Surgery, Ophthalmology, hemic and lymphatic diseases, otorhinolaryngologic diseases, Paracentesis, Medicine, Central retinal artery occlusion, Neurology (clinical), business, Clearance, Allergic granulomatous angiitis, medicine.drug
Abstract: A case of Churg Strauss syndrome (CSS) with central retinal artery occlusion is presented. This is the second fully documented case of such an event in CSS, but very probably not as a fortuitous coincidence. The patient recovered from his retinal arterial occlusion after paracentesis of the anterior eye chamber; the systemic signs and symptoms cleared slowly upon administration of corticosteroids and cyclophosphamide.
Published: 1993
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212. Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey

Author: Hou, Z., Reichardt, C. L., Story, K. T., Follin, B., Keisler, R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., de Putter, R., Dobbs, M. A., Dodelson, S., Dudley, J., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Joy, M., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., Hou, Z., Reichardt, C. L., Story, K. T., Follin, B., Keisler, R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., de Putter, R., Dobbs, M. A., Dodelson, S., Dudley, J., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Joy, M., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., and Zahn, O.
Abstract: We explore extensions to the $\Lambda$CDM cosmology using measurements of the cosmic microwave background (CMB) from the recent SPT-SZ survey, along with data from WMAP7 and measurements of $H_0$ and BAO. We check for consistency within $\Lambda$CDM between these datasets, and find some tension. The CMB alone gives weak support to physics beyond $\Lambda$CDM, due to a slight trend relative to $\Lambda$CDM of decreasing power towards smaller angular scales. While it may be due to statistical fluctuation, this trend could also be explained by several extensions. We consider running index (nrun), as well as two extensions that modify the damping tail power (the primordial helium abundance $Y_p$ and the effective number of neutrino species $N_{\rm eff}$) and one that modifies the large-scale power due to the ISW effect (the sum of neutrino masses $\sum m_\nu$). These extensions have similar observational consequences and are partially degenerate when considered simultaneously. Of the 6 one-parameter extensions considered, we find CMB to have the largest preference for nrun with -0.0460 from CMB+BAO+$H_0$+$\rm{SPT_{CL}}$. The median value is $(0.32\pm0.11)$ eV, a factor of six above the lower bound set by neutrino oscillation observations. ... [abridged], Comment: 27 pages, 20 figures. Replaced with version accepted by ApJ
Published: 2012
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213. A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey

Author: Story, K. T., Reichardt, C. L., Hou, Z., Keisler, R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., Follin, B., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Joy, M., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., Zahn, O., Story, K. T., Reichardt, C. L., Hou, Z., Keisler, R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Dudley, J., Follin, B., George, E. M., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Joy, M., Knox, L., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Millea, M., Mohr, J. J., Montroy, T. E., Padin, S., Plagge, T., Pryke, C., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Staniszewski, Z., Stark, A. A., van Engelen, A., Vanderlinde, K., Vieira, J. D., Williamson, R., and Zahn, O.
Abstract: We present a measurement of the cosmic microwave background (CMB) temperature power spectrum using data from the recently completed South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey. This measurement is made from observations of 2540 deg$^2$ of sky with arcminute resolution at $150\,$GHz, and improves upon previous measurements using the SPT by tripling the sky area. We report CMB temperature anisotropy power over the multipole range $650<\ell<3000$. We fit the SPT bandpowers, combined with the seven-year Wilkinson Microwave Anisotropy Probe (WMAP7) data, with a six-parameter LCDM cosmological model and find that the two datasets are consistent and well fit by the model. Adding SPT measurements significantly improves LCDM parameter constraints; in particular, the constraint on $\theta_s$ tightens by a factor of 2.7. The impact of gravitational lensing is detected at $8.1\, \sigma$, the most significant detection to date. This sensitivity of the SPT+WMAP7 data to lensing by large-scale structure at low redshifts allows us to constrain the mean curvature of the observable universe with CMB data alone to be $\Omega_k=-0.003^{+0.014}_{-0.018}$. Using the SPT+WMAP7 data, we measure the spectral index of scalar fluctuations to be $n_s=0.9623 \pm 0.0097$ in the LCDM model, a $3.9\,\sigma$ preference for a scale-dependent spectrum with $n_s<1$. The SPT measurement of the CMB damping tail helps break the degeneracy that exists between the tensor-to-scalar ratio $r$ and $n_s$ in large-scale CMB measurements, leading to an upper limit of $r<0.18$ (95%,C.L.) in the LCDM+$r$ model. Adding low-redshift measurements of the Hubble constant ($H_0$) and the baryon acoustic oscillation (BAO) feature to the SPT+WMAP7 data leads to further improvements. The combination of SPT+WMAP7+$H_0$+BAO constrains $n_s=0.9538 \pm 0.0081$ in the LCDM model, a $5.7\,\sigma$ detection of $n_s < 1$, ... [abridged], Comment: 21 pages, 10 figures. Replaced with version accepted by ApJ. Data products are available at http://pole.uchicago.edu/public/data/story12
Published: 2012
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214. Performance and on-sky optical characterization of the SPTpol instrument

Author: Holland, Wayne S., Zmuidzinas, Jonas, George, E. M., Lueker, M., Shirokoff, E., Vieira, J. D., Holland, Wayne S., Zmuidzinas, Jonas, George, E. M., Lueker, M., Shirokoff, E., and Vieira, J. D.
Abstract: In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camera, SPTpol, in order to measure the polarization anisotropy of the cosmic microwave background (CMB). Measurements of the polarization of the CMB at small angular scales (~several arcminutes) can detect the gravitational lensing of the CMB by large scale structure and constrain the sum of the neutrino masses. At large angular scales (~few degrees) CMB measurements can constrain the energy scale of Inflation. SPTpol is a two-color mm-wave camera that consists of 180 polarimeters at 90 GHz and 588 polarimeters at 150 GHz, with each polarimeter consisting of a dual transition edge sensor (TES) bolometers. The full complement of 150 GHz detectors consists of 7 arrays of 84 ortho-mode transducers (OMTs) that are stripline coupled to two TES detectors per OMT, developed by the TRUCE collaboration and fabricated at NIST. Each 90 GHz pixel consists of two antenna-coupled absorbers coupled to two TES detectors, developed with Argonne National Labs. The 1536 total detectors are read out with digital frequency-domain multiplexing (DfMUX). The SPTpol deployment represents the first on-sky tests of both of these detector technologies, and is one of the first deployed instruments using DfMUX readout technology. We present the details of the design, commissioning, deployment, on-sky optical characterization and detector performance of the complete SPTpol focal plane.
Published: 2012

215. Prediction of spinal epidural metastases

Author: Leo R. Canta, George E. M. Kienstra, Caroline B. Terwee, Friedo W. Dekker, Jan G.P. Tijssen, Cees C. Tijssen, D. Andries Bosch, Aernout C. W. Borstlap, Epidemiology and Data Science, AII - Inflammatory diseases, APH - Methodology, and Other departments
Subjects: Adult, Male, medicine.medical_specialty, Neurological examination, Context (language use), Myelopathy, Arts and Humanities (miscellaneous), Spinal cord compression, Risk Factors, medicine, Back pain, Humans, Medical history, Prospective Studies, Prospective cohort study, Aged, Pain Measurement, Aged, 80 and over, medicine.diagnostic_test, business.industry, Magnetic resonance imaging, Middle Aged, medicine.disease, Magnetic Resonance Imaging, Spine, Surgery, Back Pain, Female, Neurology (clinical), Radiology, Epidural Neoplasms, medicine.symptom, business, Spinal Cord Compression
Abstract: Context: Early diagnosis and treatment of spinal epidural metastases (SEM) is of the utmost importance to prevent neurological deficit due to spinal cord compression. Magnetic resonance imaging (MRI) has become the final tool in that diagnostic process. However, access to MRI is still limited in the Netherlands, requiring cost-effective use. It is generally acknowledged that patients with systemic cancer who present with a radiculopathy or myelopathy should undergo an MRI. However, the diagnostic policy in patients with systemic cancer who present with recently developed back pain is still a matter of debate. Objective: To identify the patients with back pain in whom MRI can safely be omitted because of a low risk of SEM. Methods: In a prospective series of 170 consecutive patients with cancer with recently developed back pain, prediction of spinal metastatic disease (SMD) and especially SEM was studied by means of a multivariate risk analysis of the parameters of the standard neurological evaluation (medical history, neurological examination, and plain films of the whole spine). Magnetic resonance imaging was used as the criterion standard. We calculated the risk implications of omitting MRI in patients with an estimated risk below different cutoff points. Results: Spinal metastatic disease was diagnosed in 80 patients (47%); of these, 31 had SEM. A metastatic abnormality on plain films was the strongest independent predictor for SMD. Other important predictors were night pain, progressive pain, and Karnofsky score. Advanced age, exacerbation of pain during recumbency, and osteoporotic fracture imply a low risk of SMD. Night pain and the Karnofsky score proved to be the main predictors for SEM. A plain film showing an osteoporotic fracture strongly decreased the risk of SEM. The discriminating value of the multivariate analysis was too low, and too few patients can be excluded from undergoing MRI on the basis of the standard neurological checkup. To identify all the patients with SMD (P
Published: 2000
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216. A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND DAMPING TAIL FROM THE 2500-SQUARE-DEGREE SPT-SZ SURVEY

Author: Story, K. T., primary, Reichardt, C. L., additional, Hou, Z., additional, Keisler, R., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, Follin, B., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Joy, M., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Ruhl, J. E., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2013
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217. EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg2OF THE SPT-SZ SURVEY

Author: Mocanu, L. M., primary, Crawford, T. M., additional, Vieira, J. D., additional, Aird, K. A., additional, Aravena, M., additional, Austermann, J. E., additional, Benson, B. A., additional, Béthermin, M., additional, Bleem, L. E., additional, Bothwell, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chapman, S., additional, Cho, H.-M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Everett, W. B., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Hezaveh, Y., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Rest, A., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Spieler, H. G., additional, Spilker, J. S., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K. T., additional, Switzer, E. R., additional, Vanderlinde, K., additional, and Williamson, R., additional
Published: 2013
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218. A DIRECT MEASUREMENT OF THE LINEAR BIAS OF MID-INFRARED-SELECTED QUASARS AT z ≈ 1 USING COSMIC MICROWAVE BACKGROUND LENSING

Author: Geach, J. E., primary, Hickox, R. C., additional, Bleem, L. E., additional, Brodwin, M., additional, Holder, G. P., additional, Aird, K. A., additional, Benson, B. A., additional, Bhattacharya, S., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Hainline, K. N., additional, Halverson, N. W., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Myers, A. D., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K. T., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2013
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219. Detection ofB-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope

Author: Hanson, D., primary, Hoover, S., additional, Crites, A., additional, Ade, P. A. R., additional, Aird, K. A., additional, Austermann, J. E., additional, Beall, J. A., additional, Bender, A. N., additional, Benson, B. A., additional, Bleem, L. E., additional, Bock, J. J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chiang, H. C., additional, Cho, H-M., additional, Conley, A., additional, Crawford, T. M., additional, de Haan, T., additional, Dobbs, M. A., additional, Everett, W., additional, Gallicchio, J., additional, Gao, J., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Henning, J. W., additional, Hilton, G. C., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hrubes, J. D., additional, Huang, N., additional, Hubmayr, J., additional, Irwin, K. D., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E., additional, Li, D., additional, Liang, C., additional, Luong-Van, D., additional, Marsden, G., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Montroy, T. E., additional, Natoli, T., additional, Nibarger, J. P., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Schulz, B., additional, Smecher, G., additional, Stark, A. A., additional, Story, K. T., additional, Tucker, C., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Viero, M. P., additional, Wang, G., additional, Yefremenko, V., additional, Zahn, O., additional, and Zemcov, M., additional
Published: 2013
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220. THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < 1.2 SELECTED FROM THE SPT-SZ SURVEY

Author: McDonald, M., primary, Benson, B. A., additional, Vikhlinin, A., additional, Stalder, B., additional, Bleem, L. E., additional, de Haan, T., additional, Lin, H. W., additional, Aird, K. A., additional, Ashby, M. L. N., additional, Bautz, M. W., additional, Bayliss, M., additional, Bocquet, S., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, Forman, W. R., additional, George, E. M., additional, Gettings, D., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Miller, E. D., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Nurgaliev, D., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Song, J., additional, Šuhada, R., additional, Spieler, H. G., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2013
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221. A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND

Author: Holder, G. P., primary, Viero, M. P., additional, Zahn, O., additional, Aird, K. A., additional, Benson, B. A., additional, Bhattacharya, S., additional, Bleem, L. E., additional, Bock, J., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H-M., additional, Conley, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marsden, G., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Schulz, B., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K. T., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zemcov, M., additional
Published: 2013
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222. ALMA OBSERVATIONS OF SPT-DISCOVERED, STRONGLY LENSED, DUSTY, STAR-FORMING GALAXIES

Author: Hezaveh, Y. D., primary, Marrone, D. P., additional, Fassnacht, C. D., additional, Spilker, J. S., additional, Vieira, J. D., additional, Aguirre, J. E., additional, Aird, K. A., additional, Aravena, M., additional, Ashby, M. L. N., additional, Bayliss, M., additional, Benson, B. A., additional, Bleem, L. E., additional, Bothwell, M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chapman, S. C., additional, Crawford, T. M., additional, Crites, A. T., additional, De Breuck, C., additional, de Haan, T., additional, Dobbs, M. A., additional, Fomalont, E. B., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Greve, T. R., additional, Halverson, N. W., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Husband, K., additional, Hunter, T. R., additional, Keisler, R., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Malkan, M., additional, McIntyre, V., additional, McMahon, J. J., additional, Mehl, J., additional, Menten, K. M., additional, Meyer, S. S., additional, Mocanu, L. M., additional, Murphy, E. J., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Sharon, K., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Weiß, A., additional, Welikala, N., additional, and Williamson, R., additional
Published: 2013
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223. Heme Oxygenase Inhibition Increases Blood Pressure in Pregnant Rats

Author: George, E. M., primary, Hosick, P. A., additional, Stec, D. E., additional, and Granger, J. P., additional
Published: 2013
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224. ALMA REDSHIFTS OF MILLIMETER-SELECTED GALAXIES FROM THE SPT SURVEY: THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES

Author: Weiß, A., primary, De Breuck, C., additional, Marrone, D. P., additional, Vieira, J. D., additional, Aguirre, J. E., additional, Aird, K. A., additional, Aravena, M., additional, Ashby, M. L. N., additional, Bayliss, M., additional, Benson, B. A., additional, Béthermin, M., additional, Biggs, A. D., additional, Bleem, L. E., additional, Bock, J. J., additional, Bothwell, M., additional, Bradford, C. M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chapman, S. C., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Downes, T. P., additional, Fassnacht, C. D., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Greve, T. R., additional, Halverson, N. W., additional, Hezaveh, Y. D., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Husband, K., additional, Keisler, R., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Malkan, M., additional, McIntyre, V., additional, McMahon, J. J., additional, Mehl, J., additional, Menten, K. M., additional, Meyer, S. S., additional, Murphy, E. J., additional, Padin, S., additional, Plagge, T., additional, Reichardt, C. L., additional, Rest, A., additional, Rosenman, M., additional, Ruel, J., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Spilker, J. S., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Welikala, N., additional, and Williamson, R., additional
Published: 2013
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225. Dusty starburst galaxies in the early Universe as revealed by gravitational lensing

Author: Vieira, J. D., primary, Marrone, D. P., additional, Chapman, S. C., additional, De Breuck, C., additional, Hezaveh, Y. D., additional, Weiβ, A., additional, Aguirre, J. E., additional, Aird, K. A., additional, Aravena, M., additional, Ashby, M. L. N., additional, Bayliss, M., additional, Benson, B. A., additional, Biggs, A. D., additional, Bleem, L. E., additional, Bock, J. J., additional, Bothwell, M., additional, Bradford, C. M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Fomalont, E. B., additional, Fassnacht, C. D., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Greve, T. R., additional, Gullberg, B., additional, Halverson, N. W., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Hunter, T. R., additional, Keisler, R., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Malkan, M., additional, McIntyre, V., additional, McMahon, J. J., additional, Mehl, J., additional, Menten, K. M., additional, Meyer, S. S., additional, Mocanu, L. M., additional, Murphy, E. J., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Sharon, K., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spilker, J. S., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Welikala, N., additional, and Williamson, R., additional
Published: 2013
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226. 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, B. A., primary, de Haan, T., additional, Dudley, J. P., additional, Reichardt, C. L., additional, Aird, K. A., additional, Andersson, K., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bayliss, M., additional, Bazin, G., additional, Bleem, L. E., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, Desai, S., additional, Dobbs, M. A., additional, Foley, R. J., additional, Forman, W. R., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, Suhada, R., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2013
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227. GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL’DOVICH EFFECT IN THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY

Author: Reichardt, C. L., primary, Stalder, B., additional, Bleem, L. E., additional, Montroy, T. E., additional, Aird, K. A., additional, Andersson, K., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bayliss, M., additional, Bazin, G., additional, Benson, B. A., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, Forman, W. R., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N. L., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Murray, S. S., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, Šuhada, R., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2013
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228. SPT-CL J0205–5829: Az= 1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY

Author: Stalder, B., primary, Ruel, J., additional, Šuhada, R., additional, Brodwin, M., additional, Aird, K. A., additional, Andersson, K., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bayliss, M., additional, Bazin, G., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, Forman, W. R., additional, George, E. M., additional, Gettings, D., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N. L., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Natoli, T., additional, Nurgaliev, D., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2013
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229. MULTIFIDELITY INFORMATION FUSION ALGORITHMS FOR HIGH-DIMENSIONAL SYSTEMS AND MASSIVE DATA SETS.

Author: PERDIKARIS, PARIS, VENTURI, DANIELE, and KARNIADAKIS, GEORGE E. M.
Subjects: FUSION (Phase transformation), GAUSSIAN processes, MULTIVARIATE analysis, ANALYSIS of variance, DISTRIBUTION (Probability theory), MATHEMATICAL models
Abstract: We develop a framework for multifidelity information fusion and predictive inference in high-dimensional input spaces and in the presence of massive data sets. Hence, we tackle simultaneously the "big N" problem for big data and the curse of dimensionality in multivariate parametric problems. The proposed methodology establishes a new paradigm for constructing response surfaces of high-dimensional stochastic dynamical systems, simultaneously accounting for multifidelity in physical models as well as multifidelity in probability space. Scaling to high dimensions is achieved by data-driven dimensionality reduction techniques based on hierarchical functional decompositions and a graph-theoretic approach for encoding custom autocorrelation structure in Gaussian process priors. Multifidelity information fusion is facilitated through stochastic autoregressive schemes and frequency-domain machine learning algorithms that scale linearly with the data. Taking together these new developments leads to linear complexity algorithms as demonstrated in benchmark problems involving deterministic and stochastic fields in up to 105 input dimensions and 105 training points on a standard desktop computer. [ABSTRACT FROM AUTHOR]
Published: 2016
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230. HIGH-REDSHIFT COOL-CORE GALAXY CLUSTERS DETECTED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE SOUTH POLE TELESCOPE SURVEY

Author: Semler, D. R., primary, Šuhada, R., additional, Aird, K. A., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bayliss, M., additional, Bazin, G., additional, Bocquet, S., additional, Benson, B. A., additional, Bleem, L. E., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N. L., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2012
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231. REDSHIFTS, SAMPLE PURITY, AND BCG POSITIONS FOR THE GALAXY CLUSTER CATALOG FROM THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY

Author: Song, J., primary, Zenteno, A., additional, Stalder, B., additional, Desai, S., additional, Bleem, L. E., additional, Aird, K. A., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bayliss, M., additional, Bazin, G., additional, Benson, B. A., additional, Bertin, E., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, George, E. M., additional, Gettings, D., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N. L., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Nurgaliev, D., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Šuhada, R., additional, Spieler, H. G., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2012
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232. Feedhorn-coupled TES polarimeter camera modules at 150 GHz for CMB polarization measurements with SPTpol

Author: Henning, J. W., primary, Ade, P., additional, Aird, K. A., additional, Austermann, J. E., additional, Beall, J. A., additional, Becker, D., additional, Benson, B. A., additional, Bleem, L. E., additional, Britton, J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, Datesman, A., additional, de Haan, T., additional, Dobbs, M A., additional, Everett, W., additional, Ewall-Wice, A., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Hilton, G. C., additional, Holzapfel, W. L., additional, Hubmayr, J., additional, Irwin, K. D., additional, Karfunkle, M., additional, Keisler, R., additional, Kennedy, J., additional, Lee, A. T., additional, Leitch, E., additional, Li, D., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montgomery, J., additional, Montroy, T. E., additional, Nagy, J., additional, Natoli, T., additional, Nibarger, J. P., additional, Niemack, M. D., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Story, K., additional, Tucker, C., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wang, G., additional, Williamson, R., additional, Yefremenko, V., additional, Yoon, K. W., additional, and Young, E., additional
Published: 2012
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233. Design and characterization of 90 GHz feedhorn-coupled TES polarimeter pixels in the SPTPol camera

Author: Sayre, J. T., primary, Ade, P., additional, Aird, K. A., additional, Austermann, J. E., additional, Beall, J. A., additional, Becker, D., additional, Benson, B. A., additional, Bleem, L. E., additional, Britton, J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, Datesman, A., additional, de Haan, T., additional, Dobbs, M. A., additional, Everett, W., additional, Ewall-Wice, A., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Henning, J. W., additional, Hilton, G. C., additional, Holzapfel, W. L., additional, Hubmayr, J., additional, Irwin, K. D., additional, Karfunkle, M., additional, Keisler, R., additional, Kennedy, J., additional, Lee, A. T., additional, Leitch, E., additional, Li, D., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montgomery, J., additional, Montroy, T. E., additional, Nagy, J., additional, Natoli, T., additional, Nibarger, J. P., additional, Niemack, M. D., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Story, K., additional, Tucker, C., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wang, G., additional, Williamson, R., additional, Yefremenko, V., additional, Yoon, K. W., additional, and Young, E., additional
Published: 2012
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234. SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope

Author: Austermann, J. E., primary, Aird, K. A., additional, Beall, J. A., additional, Becker, D., additional, Bender, A., additional, Benson, B. A., additional, Bleem, L. E., additional, Britton, J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chiang, H. C., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, Datesman, A., additional, de Haan, T., additional, Dobbs, M. A., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Henning, J. W., additional, Hilton, G. C., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Huang, N., additional, Hubmayr, J., additional, Irwin, K. D., additional, Keisler, R., additional, Kennedy, J., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E., additional, Li, D., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montroy, T. E., additional, Natoli, T., additional, Nibarger, J. P., additional, Niemack, M. D., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wang, G., additional, Williamson, R., additional, Yefremenko, V., additional, Yoon, K. W., additional, and Zahn, O., additional
Published: 2012
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235. WEAK-LENSING MASS MEASUREMENTS OF FIVE GALAXY CLUSTERS IN THE SOUTH POLE TELESCOPE SURVEY USING MAGELLAN/MEGACAM

Author: High, F. W., primary, Hoekstra, H., additional, Leethochawalit, N., additional, de Haan, T., additional, Abramson, L., additional, Aird, K. A., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bayliss, M., additional, Bazin, G., additional, Benson, B. A., additional, Bleem, L. E., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Clocchiatti, A., additional, Conroy, M., additional, Crawford, T. M., additional, Crites, A. T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, Forman, W. R., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N. L., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Liu, J., additional, Lueker, M., additional, Luong-Van, D., additional, Mantz, A., additional, Marrone, D. P., additional, McDonald, M., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mocanu, L., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Natoli, T., additional, Nurgaliev, D., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Schrabback, T., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, Šuhada, R., additional, Tokarz, S., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2012
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236. Performance and on-sky optical characterization of the SPTpol instrument

Author: George, E. M., primary, Ade, P., additional, Aird, K. A., additional, Austermann, J. E., additional, Beall, J. A., additional, Becker, D., additional, Bender, A., additional, Benson, B. A., additional, Bleem, L. E., additional, Britton, J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chiang, H. C., additional, Cho, H.-M., additional, Crawford, T. M., additional, Crites, A. T., additional, Datesman, A., additional, de Haan, T., additional, Dobbs, M. A., additional, Everett, W., additional, Ewall-Wice, A., additional, Halverson, N. W., additional, Harrington, N., additional, Henning, J. W., additional, Hilton, G. C., additional, Holzapfel, W. L., additional, Hoover, S., additional, Huang, N., additional, Hubmayr, J., additional, Irwin, K. D., additional, Karfunkle, M., additional, Keisler, R., additional, Kennedy, J., additional, Lee, A. T., additional, Leitch, E., additional, Li, D., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montgomery, J., additional, Montroy, T. E., additional, Nagy, J., additional, Natoli, T., additional, Nibarger, J. P., additional, Niemack, M. D., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Story, K., additional, Tucker, C., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wang, G., additional, Williamson, R., additional, Yefremenko, V., additional, Yoon, K. W., additional, and Young, E., additional
Published: 2012
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237. South Pole Telescope software systems: control, monitoring, and data acquisition

Author: Story, K., primary, Leitch, E., additional, Ade, P., additional, Aird, K. A., additional, Austermann, J. E., additional, Beall, J. A., additional, Becker, D., additional, Bender, A. N., additional, Benson, B. A., additional, Bleem, L. E., additional, Britton, J., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chiang, H. C., additional, Cho, H-M., additional, Crawford, T. M., additional, Crites, A. T., additional, Datesman, A., additional, de Haan, T., additional, Dobbs, M. A., additional, Everett, W., additional, Ewall-Wice, A., additional, George, E. M., additional, Halverson, N. W., additional, Harrington, N., additional, Henning, J. W., additional, Hilton, G. C., additional, Holzapfel, W. L., additional, Hoover, S., additional, Huang, N., additional, Hubmayr, J., additional, Irwin, K. D., additional, Karfunkle, M., additional, Keisler, R., additional, Kennedy, J., additional, Lee, A. T., additional, Li, D., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montgomery, J., additional, Montroy, T. E., additional, Nagy, J., additional, Natoli, T., additional, Nibarger, J. P., additional, Niemack, M. D., additional, Novosad, V., additional, Padin, S., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Smecher, G., additional, Stalder, B., additional, Tucker, C., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wang, G., additional, Williamson, R., additional, Yefremenko, V., additional, Yoon, K. W., additional, and Young, E., additional
Published: 2012
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238. A MEASUREMENT OF GRAVITATIONAL LENSING OF THE MICROWAVE BACKGROUND USING SOUTH POLE TELESCOPE DATA

Author: van Engelen, A., primary, Keisler, R., additional, Zahn, O., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Joy, M., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Vieira, J. D., additional, and Williamson, R., additional
Published: 2012
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239. SUBMILLIMETER OBSERVATIONS OF MILLIMETER BRIGHT GALAXIES DISCOVERED BY THE SOUTH POLE TELESCOPE

Author: Greve, T. R., primary, Vieira, J. D., additional, Weiß, A., additional, Aguirre, J. E., additional, Aird, K. A., additional, Ashby, M. L. N., additional, Benson, B. A., additional, Bleem, L. E., additional, Bradford, C. M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chapman, S. C., additional, Crawford, T. M., additional, de Breuck, C., additional, de Haan, T., additional, Dobbs, M. A., additional, Downes, T., additional, Fassnacht, C. D., additional, Fazio, G., additional, George, E. M., additional, Gladders, M., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Hezaveh, Y., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Johnson, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Malkan, M., additional, Marrone, D. P., additional, McIntyre, V., additional, McMahon, J. J., additional, Mehl, J., additional, Menten, K. M., additional, Meyer, S. S., additional, Montroy, T., additional, Murphy, E. J., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Rosenman, M., additional, Ruel, J., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Sharon, K., additional, Shaw, L., additional, Shirokoff, E., additional, Stalder, B., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Walsh, W., additional, Welikala, N., additional, and Williamson, R., additional
Published: 2012
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240. COSMIC MICROWAVE BACKGROUND CONSTRAINTS ON THE DURATION AND TIMING OF REIONIZATION FROM THE SOUTH POLE TELESCOPE

Author: Zahn, O., primary, Reichardt, C. L., additional, Shaw, L., additional, Lidz, A., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Doré, O., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, and Williamson, R., additional
Published: 2012
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241. A MEASUREMENT OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH TWO YEARS OF SOUTH POLE TELESCOPE OBSERVATIONS

Author: Reichardt, C. L., primary, Shaw, L., additional, Zahn, O., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, and Williamson, R., additional
Published: 2012
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242. Frequency multiplexed superconducting quantum interference device readout of large bolometer arrays for cosmic microwave background measurements

Author: Dobbs, M. A., primary, Lueker, M., additional, Aird, K. A., additional, Bender, A. N., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H.-M., additional, Clarke, J., additional, Crawford, T. M., additional, Crites, A. T., additional, Flanigan, D. I., additional, de Haan, T., additional, George, E. M., additional, Halverson, N. W., additional, Holzapfel, W. L., additional, Hrubes, J. D., additional, Johnson, B. R., additional, Joseph, J., additional, Keisler, R., additional, Kennedy, J., additional, Kermish, Z., additional, Lanting, T. M., additional, Lee, A. T., additional, Leitch, E. M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Richards, P. L., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Schwan, D., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vu, C., additional, Westbrook, B., additional, and Williamson, R., additional
Published: 2012
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243. A MEASUREMENT OF THE CORRELATION OF GALAXY SURVEYS WITH CMB LENSING CONVERGENCE MAPS FROM THE SOUTH POLE TELESCOPE

Author: Bleem, L. E., primary, van Engelen, A., additional, Holder, G. P., additional, Aird, K. A., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Becker, M. R., additional, Benson, B. A., additional, Biesiadzinski, T., additional, Brodwin, M., additional, Busha, M. T., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Doré, O., additional, Dudley, J., additional, Geach, J. E., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Harrington, N., additional, High, F. W., additional, Holden, B. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, Martinez-Manso, J., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sayre, J. T., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Stalder, B., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Stern, D., additional, Story, K., additional, Vallinotto, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Wechsler, R. H., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2012
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244. THE FIRST PUBLIC RELEASE OF SOUTH POLE TELESCOPE DATA: MAPS OF A 95 deg2FIELD FROM 2008 OBSERVATIONS

Author: Schaffer, K. K., primary, Crawford, T. M., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Ruhl, J. E., additional, Shirokoff, E., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Vieira, J. D., additional, and Williamson, R., additional
Published: 2011
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245. A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE

Author: Keisler, R., primary, Reichardt, C. L., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hou, Z., additional, Hrubes, J. D., additional, Joy, M., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Millea, M., additional, Mohr, J. J., additional, Montroy, T. E., additional, Natoli, T., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, van Engelen, A., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2011
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246. Endothelin: Key Mediator of Hypertension in Preeclampsia

Author: George, E. M., primary and Granger, J. P., additional
Published: 2011
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247. A SUNYAEV-ZEL'DOVICH-SELECTED SAMPLE OF THE MOST MASSIVE GALAXY CLUSTERS IN THE 2500 deg2SOUTH POLE TELESCOPE SURVEY

Author: Williamson, R., primary, Benson, B. A., additional, High, F. W., additional, Vanderlinde, K., additional, Ade, P. A. R., additional, Aird, K. A., additional, Andersson, K., additional, Armstrong, R., additional, Ashby, M. L. N., additional, Bautz, M., additional, Bazin, G., additional, Bertin, E., additional, Bleem, L. E., additional, Bonamente, M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Chapman, S. C., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Fazio, G. G., additional, Foley, R. J., additional, Forman, W. R., additional, Garmire, G., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Stanford, S. A., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Stubbs, C. W., additional, Vieira, J. D., additional, Vikhlinin, A., additional, and Zenteno, A., additional
Published: 2011
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248. X-RAY PROPERTIES OF THE FIRST SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTER SAMPLE FROM THE SOUTH POLE TELESCOPE

Author: Andersson, K., primary, Benson, B. A., additional, Ade, P. A. R., additional, Aird, K. A., additional, Armstrong, B., additional, Bautz, M., additional, Bleem, L. E., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, Forman, W. R., additional, Garmire, G., additional, George, E. M., additional, Gladders, M. D., additional, Halverson, N. W., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hrubes, J. D., additional, Jones, C., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Murray, S. S., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Stubbs, C. W., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Vikhlinin, A., additional, Williamson, R., additional, Yang, Y., additional, Zahn, O., additional, and Zenteno, A., additional
Published: 2011
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249. IMPROVED CONSTRAINTS ON COSMIC MICROWAVE BACKGROUND SECONDARY ANISOTROPIES FROM THE COMPLETE 2008 SOUTH POLE TELESCOPE DATA

Author: Shirokoff, E., primary, Reichardt, C. L., additional, Shaw, L., additional, Millea, M., additional, Ade, P. A. R., additional, Aird, K. A., additional, Benson, B. A., additional, Bleem, L. E., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Cho, H. M., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Dobbs, M. A., additional, Dudley, J., additional, George, E. M., additional, Halverson, N. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Ruhl, J. E., additional, Schaffer, K. K., additional, Spieler, H. G., additional, Staniszewski, Z., additional, Stark, A. A., additional, Story, K., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zahn, O., additional
Published: 2011
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250. SOUTH POLE TELESCOPE DETECTIONS OF THE PREVIOUSLY UNCONFIRMED PLANCK EARLY SUNYAEV-ZEL’DOVICH CLUSTERS IN THE SOUTHERN HEMISPHERE

Author: Story, K., primary, Aird, K. A., additional, Andersson, K., additional, Armstrong, R., additional, Bazin, G., additional, Benson, B. A., additional, Bleem, L. E., additional, Bonamente, M., additional, Brodwin, M., additional, Carlstrom, J. E., additional, Chang, C. L., additional, Clocchiatti, A., additional, Crawford, T. M., additional, Crites, A. T., additional, de Haan, T., additional, Desai, S., additional, Dobbs, M. A., additional, Dudley, J. P., additional, Foley, R. J., additional, George, E. M., additional, Gladders, M. D., additional, Gonzalez, A. H., additional, Halverson, N. W., additional, High, F. W., additional, Holder, G. P., additional, Holzapfel, W. L., additional, Hoover, S., additional, Hrubes, J. D., additional, Joy, M., additional, Keisler, R., additional, Knox, L., additional, Lee, A. T., additional, Leitch, E. M., additional, Lueker, M., additional, Luong-Van, D., additional, Marrone, D. P., additional, McMahon, J. J., additional, Mehl, J., additional, Meyer, S. S., additional, Mohr, J. J., additional, Montroy, T. E., additional, Padin, S., additional, Plagge, T., additional, Pryke, C., additional, Reichardt, C. L., additional, Rest, A., additional, Ruel, J., additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Saro, A., additional, Schaffer, K. K., additional, Shaw, L., additional, Shirokoff, E., additional, Song, J., additional, Spieler, H. G., additional, Stalder, B., additional, Staniszewski, Z., additional, Stark, A. A., additional, Stubbs, C. W., additional, Vanderlinde, K., additional, Vieira, J. D., additional, Williamson, R., additional, and Zenteno, A., additional
Published: 2011
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