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23 April 2024
 
  » arxiv » astro-ph/0012282

 Article overview


AMiBA: Array for Microwave Background Anisotropy
K. Y. Lo ; T. H. Chiueh ; R. N. Martin ; Kin-Wang Ng ; H. Liang ; Ue-li Pen ; Chung-Pei Ma ;
Date 13 Dec 2000
Subject astro-ph
Affiliation1,2), T. H. Chiueh (2,1), R. N. Martin , Kin-Wang Ng , H. Liang , Ue-li Pen (4,1), Chung-Pei Ma (5,1) (ASIAA National Taiwan University University of Bristol CITA U. Penn
AbstractAs part of a 4-year Cosmology and Particle Astrophysics (CosPA) Research Excellence Initiative in Taiwan, AMiBA $-$ a 19-element dual-channel 85-105 GHz interferometer array is being specifically built to search for high redshift clusters of galaxies via the Sunyaev-Zeldovich Effect (SZE). In addition, AMiBA will have full polarization capabilities, in order to probe the polarization properties of the Cosmic Microwave Background. AMiBA, to be sited on Mauna Kea in Hawaii or in Chile, will reach a sensitivity of $sim 1$ mJy or 7$mu$K in 1 hour. The project involves extensive international scientific and technical collaborations. The construction of AMiBA is scheduled to starting operating in early 2004.
Source arXiv, astro-ph/0012282
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