Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups

Autor: Liu, J., Mohr, J., Saro, A., Aird, K. A., Ashby, M. L. N., Bautz, M., Bayliss, M., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dietrich, J. P., Dobbs, M. A., Foley, R. J., Gangkofner, D., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Hlavacek-Larrondo, J., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McDonald, M., McMahon, J. J., Meyer, S. S., Mocanu, L., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Spieler, H. G., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Suhada, R., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., Zenteno, A.

Publikováno v: MNRAS (April 11, 2015) 448 (3): 2085-2099

(Abridged) We use 95, 150, and 220GHz observations from the SPT to examine the SZE signatures of a sample of 46 X-ray selected groups and clusters drawn from ~6 deg^2 of the XMM-BCS. These systems extend to redshift z=1.02, have characteristic masses

Externí odkaz: http://arxiv.org/abs/1407.7520

Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope

Autor: Saro, A., Liu, J., Mohr, J. J., Aird, K. A., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dietrich, J. P., Dobbs, M. A., Dolag, K., Dudley, J. P., Foley, R. J., Gangkofner, D., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McDonald, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., Murray, S. S., Nurgaliev, D., Padin, S., Patej, A., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Spieler, H. G., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., Zenteno, A.

The adiabatic evolution of the temperature of the cosmic microwave background (CMB) is a key prediction of standard cosmology. We study deviations from the expected adiabatic evolution of the CMB temperature of the form $T(z) =T_0(1+z)^{1-\alpha}$ us

Externí odkaz: http://arxiv.org/abs/1312.2462

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The dark energy survey and operations: years 1 to 3

Autor: Peck, Alison B., Seaman, Robert L., Benn, Chris R., Diehl, H. T., Neilsen, E., Gruendl, R., Yanny, B., Abbott, T. M. C., Aleksić, J., Allam, S., Annis, J., Balbinot, E., Baumer, M., Beaufore, L., Bechtol, K., Bernstein, G., Birrer, S., Bonnett, C., Brout, D., Bruderer, C., Buckley-Geer, E. J., Capozzi, D., Carnero Rosell, A., Castander, F. J., Cawthon, R., Chang, C., Clerkin, L., Covarrubias, R., Cuhna, C., D'Andrea, C., da Costa, L., Das, R., Davis, C., Dietrich, J., Drlica-Wagner, A., Elliott, A., Eifler, T. F., Etherington, J., Flaugher, B. L., Frieman, J., Fausti Neto, A., Fernández, M. G., Furlanetto, C., Gangkofner, D., Gerdes, D. W., Goldstein, D. A., Grabowski, K., Gupta, R. R., Hamilton, S., Head, H., Helsby, J., Hollowood, D., Honscheid, K., James, D., Johnson, M., Johnson, M. W. G., Jouvel, S., Kacprzac, T., Kent, S., Kessler, R., Kim, A., Krause, E., Krawiec, C. I., Kremin, A., Kron, R., Kuhlmann, S., Kuropatkin, N., Lahav, O., Lasker, J., Li, T. S., Luque, E., Maccrann, N., March, M., Marshall, J., Mondrik, N. P., Morganson, E. P., Mudd, D., Nadolski, A., Nugent, P., Melchior, P., Menanteau, F., Nagasawa, D. Q., Nord, B., Ogando, R., Old, L., Palmese, A., Petravick, D., Plazas, A. A., Pujol, A., Queiroz, A. B. A., Reil, K., Romer, A. K., Rosenfeld, R., Roodman, A., Rooney, P., Sako, M., Salvador, A. I., Sánchez, C., Sánchez Álvaro, E., Santiago, B. X., Schooneveld, A., Schubnell, M., Sheldon, E., Smith, A., Smith, R. C., Soares-Santos, M., Sobreira, F., Soumagnac, M., Spinka, H., Tie, S. S., Tucker, D., Vikram, V., Vivas, K., Walker, A. R., Wester, W., Wiesner, M., Wilcox, H., Williams, P., Zenteno, A., Zhang, Y., Zhang, Z.

Publikováno v: Proceedings of SPIE; August 2016, Vol. 9910 Issue: 1 p99101D-99101D-19, 9811019p

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