paper

A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey

arXiv:1210.7231 · doi:10.1088/0004-637X/779/1/86

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 of sky with arcminute resolution at GHz, and improves upon previous measurements using the SPT by tripling the sky area. We report CMB temperature anisotropy power over the multipole range . 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 tightens by a factor of 2.7. The impact of gravitational lensing is detected at , 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 . Using the SPT+WMAP7 data, we measure the spectral index of scalar fluctuations to be in the LCDM model, a preference for a scale-dependent spectrum with . The SPT measurement of the CMB damping tail helps break the degeneracy that exists between the tensor-to-scalar ratio and in large-scale CMB measurements, leading to an upper limit of (95%,C.L.) in the LCDM+ model. Adding low-redshift measurements of the Hubble constant () and the baryon acoustic oscillation (BAO) feature to the SPT+WMAP7 data leads to further improvements. The combination of SPT+WMAP7++BAO constrains in the LCDM model, a detection of , ... [abridged]

21 pages, 10 figures. Replaced with version accepted by ApJ. Data products are available at http://pole.uchicago.edu/public/data/story12/