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AMiBA: Array for Microwave Background Anisotropy

Published online by Cambridge University Press:  26 May 2016

K. Y. Lo ,
T. H. Chiueh ,
R. N. Martin ,
Kin-Wang Ng ,
H. Liang ,
Ue-Li Pen  and
Chung-Pei Ma
K. Y. Lo
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) and Physics department, National Taiwan University (NTU)
T. H. Chiueh
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) and Physics department, National Taiwan University (NTU)
R. N. Martin
Affiliation:
ASIAA
Kin-Wang Ng
Affiliation:
ASIAA
H. Liang
Affiliation:
Physics department, University of Bristol
Ue-Li Pen
Affiliation:
Canadian Institute of Theoretical Astrophysics (CITA) and ASIAA
Chung-Pei Ma
Affiliation:
Physics department, University of Pennsylvania and ASIAA

Abstract

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As 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 ˜ 1 mJy or 7μK in 1 hour. The project involves extensive international scientific and technical collaborations. The construction of AMiBA is scheduled to starting operating in early 2004.

Type
Part VIII: Dark Matter and Ω0
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 306 - 311
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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