201. Optical spectroscopy and velocity dispersions of galaxy clusters from the SPT-SZ survey
- Author
-
Mark Brodwin, M. L. N. Ashby, Armin Rest, Adrian T. Lee, Lloyd Knox, S. A. Stanford, Marshall Joy, Christopher W. Stubbs, J. P. Dudley, J. Song, T. Natoli, W. L. Holzapfel, J. T. Sayre, K. Vanderlinde, Jeff McMahon, Ryan J. Foley, Scott Chapman, Adam Mantz, Sebastian Bocquet, K. A. Aird, Matt Dobbs, Elizabeth George, Robert Armstrong, Matthew B. Bayliss, Michael McDonald, William R. Forman, S. S. Murray, T. M. Crawford, Joseph J. Mohr, K. K. Schaffer, J. Mehl, A. Saro, Marshall W. Bautz, R. Suhada, B. Stalder, N. W. Halverson, Benjamin Saliwanchik, T. E. Montroy, Gilbert Holder, M. Lueker, A. Clocchiatti, A. van Engelen, Christian L. Reichardt, D. Nurgaliev, Stephen Padin, O. Zahn, Alfredo Zenteno, Michael D. Gladders, Antony A. Stark, Erik Shirokoff, C. Jones, J. D. Hrubes, Anthony H. Gonzalez, Joaquin Vieira, Lindsey Bleem, S. S. Meyer, A. T. Crites, S. Desai, C. Pryke, E. M. Leitch, R. Williamson, J. E. Ruhl, H. M. Cho, Ryan Keisler, Alexey Vikhlinin, G. Bazin, T. Plagge, Z. Staniszewski, Helmuth Spieler, L. M. Mocanu, Daniel P. Marrone, L. Shaw, F. W. High, Jonathan Ruel, Daniel M. Luong-Van, Bradford Benson, C. L. Chang, N. L. Harrington, John E. Carlstrom, T. de Haan, K. T. Story, Jiayi Liu, Ruel, J., Bazin, G., Bayliss, M., Brodwin, M., Foley, R. J., Stalder, B., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bautz, M., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Chapman, S. C., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., De Haan, T., Desai, S., Dobbs, M. A., Dudley, J. P., Forman, W. R., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Harrington, N. L., High, F. W., Holder, G. P., Holzapfel, W. L., 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., Mcdonald, M., Mcmahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Natoli, T., Nurgaliev, D., 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., Shaw, L., Shirokoff, E., Song, J., Šuhada, R., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Starsk, A. A., Story, K., Stubbs, C. W., Van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Physics ,catalog ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Velocity dispersion ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Astronomy and Astrophysic ,Galaxy ,Redshift ,South Pole Telescope ,galaxies: clusters: general ,Space and Planetary Science ,Cluster (physics) ,clusters: general [galaxies] ,Spectroscopy ,Scaling ,catalogs ,Galaxy cluster ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present optical spectroscopy of galaxies in clusters detected through the Sunyaev-Zel'dovich (SZ) effect with the South Pole Telescope (SPT). We report our own measurements of $61$ spectroscopic cluster redshifts, and $48$ velocity dispersions each calculated with more than $15$ member galaxies. This catalog also includes $19$ dispersions of SPT-observed clusters previously reported in the literature. The majority of the clusters in this paper are SPT-discovered; of these, most have been previously reported in other SPT cluster catalogs, and five are reported here as SPT discoveries for the first time. By performing a resampling analysis of galaxy velocities, we find that unbiased velocity dispersions can be obtained from a relatively small number of member galaxies ($\lesssim 30$), but with increased systematic scatter. We use this analysis to determine statistical confidence intervals that include the effect of membership selection. We fit scaling relations between the observed cluster velocity dispersions and mass estimates from SZ and X-ray observables. In both cases, the results are consistent with the scaling relation between velocity dispersion and mass expected from dark-matter simulations. We measure a $\sim$30% log-normal scatter in dispersion at fixed mass, and a $\sim$10% offset in the normalization of the dispersion-mass relation when compared to the expectation from simulations, which is within the expected level of systematic uncertainty., Comment: Accepted to ApJ. 20 pages, 6 figures
- Published
- 2014