The Atacama Cosmology Telescope: Cosmology from Galaxy Clusters Detected via the Sunyaev-Zel'dovich Effect
Creators: name: Sehgal, Neelima
name: Trac, Hy
name: Acquaviva, Viviana
name: Ade, Peter A. R.
name: Aguirre, Paula
name: Amiri, Mandana
name: Appel, John W.
name: Barrientos, L. Felipe
name: Battistelli, Elia S.
name: Bond, J. Richard
name: Brown, Ben
name: Burger, Bryce
name: Chervenak, Jay
name: Das, Sudeep
name: Devlin, Mark J.
name: Dicker, Simon R.
name: Doriese, W. Bertrand
name: Dunkley, Joanna
name: Dünner, Rolando
name: Essinger-Hileman, Thomas
name: Fisher, Ryan P.
name: Fowler, Joseph W.
name: Hajian, Amir
name: Halpern, Mark
name: Hasselfield, Matthew
name: Hernández-Monteagudo, Carlos
name: Hilton, Gene C.
name: Hilton, Matt
name: Hincks, Adam D.
name: Hlozek, Renée
name: Holtz, David
name: Huffenberger, Kevin M.
name: Hughes, David H.
name: Hughes, John P.
name: Infante, Leopoldo
name: Irwin, Kent D.
name: Jones, Andrew
name: Juin, Jean Baptiste
name: Klein, Jeff
name: Kosowsky, Arthur
name: Lau, Judy M.
name: Limon, Michele
name: Lin, Yen-Ting
name: Lupton, Robert H.
name: Marriage, Tobias A.
name: Marsden, Danica
name: Martocci, Krista
name: Mauskopf, Phil
name: Menanteau, Felipe
name: Moodley, Kavilan
name: Moseley, Harvey
name: Netterfield, Calvin B.
name: Niemack, Michael D.
name: Nolta, Michael R.
name: Page, Lyman A.
name: Parker, Lucas
name: Partridge, Bruce
name: Reid, Beth
name: Sherwin, Blake D.
name: Sievers, Jon
name: Spergel, David N.
name: Staggs, Suzanne T.
name: Swetz, Daniel S.
name: Switzer, Eric R.
name: Thornton, Robert
name: Tucker, Carole
name: Warne, Ryan
name: Wollack, Ed
name: Zhao, Yue
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We present constraints on cosmological parameters based on a sample of Sunyaev-Zel'dovich-selected galaxy clusters detected in a millimeter-wave survey by the Atacama Cosmology Telescope. The cluster sample used in this analysis consists of 9 optically-confirmed high-mass clusters comprising the high-significance end of the total cluster sample identified in 455 square degrees of sky surveyed during 2008 at 148 GHz. We focus on the most massive systems to reduce the degeneracy between unknown cluster astrophysics and cosmology derived from SZ surveys. We describe the scaling relation between cluster mass and SZ signal with a 4-parameter fit. Marginalizing over the values of the parameters in this fit with conservative priors gives sigma_8 = 0.851 +/- 0.115 and w = -1.14 +/- 0.35 for a spatially-flat wCDM cosmological model with WMAP 7-year priors on cosmological parameters. This gives a modest improvement in statistical uncertainty over WMAP 7-year constraints alone. Fixing the scaling relation between cluster mass and SZ signal to a fiducial relation obtained from numerical simulations and calibrated by X-ray observations, we find sigma_8 = 0.821 +/- 0.044 and w = -1.05 +/- 0.20. These results are consistent with constraints from WMAP 7 plus baryon acoustic oscillations plus type Ia supernoava which give sigma_8 = 0.802 +/- 0.038 and w = -0.98 +/- 0.053. A stacking analysis of the clusters in this sample compared to clusters simulated assuming the fiducial model also shows good agreement. These results suggest that, given the sample of clusters used here, both the astrophysics of massive clusters and the cosmological parameters derived from them are broadly consistent with current models.
description: 12 pages, 7 figures. Submitted to ApJ