First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: Abell 3266

P.L. Gomez , A.K. Romer , J.B. Peterson (1) , C.M. Cantalupo (1 , 2) , S.W.L. Holzapfel , C.L. Kuo , M. Newcomb (3)

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J. Ruhl (4) J. Goldstein E. Torbet (5) M.C. Runyan (6) ((1) CMU (2) LBNL (3) UC Berkeley (4) CWRU (5) UCSB (6) Caltech)

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classification 🌌 astro-ph

keywords x-rayclustersabellacbaranisotropiesbackgroundcosmiceffect

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As part of a combined Sunyaev-Zeldovich Effect (SZE), X-ray and weak lensing survey of low redshift (z<0.1) X-ray clusters, we present SZE images of the z=0.059 X-ray cluster Abell 3266 at three observing frequencies (150, 220, 275 GHz) and after the spectral subtraction of primary Cosmic Microwave Background (CMB) anisotropies. These images were generated using the ACBAR bolometer array operated on the Viper telescope at the South Pole. The multi-frequency data from ACBAR should allow us to overcome one of the main obstacles facing the analysis of SZE observations of nearby clusters, i.e. contamination from primary Cosmic Microwave Background (CMB) anisotropies.

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First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: Abell 3266

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