Journal
PHYSICAL REVIEW D
Volume 86, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.86.122005
Keywords
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Funding
- U.S. NSF [AST-0408698, PHY-0355328, AST-0707731, PIRE-0507768]
- Princeton University
- University of Pennsylvania
- FONDAP
- Basal, Centre AIUC
- RCUK Fellowship
- NASA [NNX08AH30G]
- NSERC PGSD
- NSF [AST-0546035, AST-0807790]
- NSF PFC [PHY-0114422]
- KICP Fellowship
- SLAC [DE-AC3-76SF00515]
- ERC [259505]
- BCCP
- NSF GRFP
- Programa de Astronomia, a program of the Comision Nacional de Investigacion Cientifica y Tecnologica de Chile (CONICYT)
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1102762] Funding Source: National Science Foundation
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We present a detection of the unnormalized skewness <(T) over tilde (3)((n) over cap)> induced by the thermal Sunyaev-Zel'dovich (tSZ) effect in filtered Atacama Cosmology Telescope ( ACT) 148 GHz cosmic microwave background temperature maps. Contamination due to infrared and radio sources is minimized by template subtraction of resolved sources and by constructing a mask using outlying values in the 218 GHz (tSZ-null) ACT maps. We measure <(T) over tilde (3)((n) over cap)> = -31 +/- 6 mu K-3 (Gaussian statistics assumed) or +/- 14 mu K-3 ( including non- Gaussian corrections) in the filtered ACT data, a 5 sigma detection. We show that the skewness is a sensitive probe of sigma(8), and use analytic calculations and tSZ simulations to obtain cosmological constraints from this measurement. From this signal alone we infer a value of sigma(8) = 0.79(-0.03)(+0.03) (68% C.L.) (+0.06)(-0.06)(95% C.L.). Our results demonstrate that measurements of non- Gaussianity can be a useful method for characterizing the tSZ effect and extracting the underlying cosmological information. DOI: 10.1103/PhysRevD.86.122005
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