AMiBA: Array for Microwave Background Anisotropy

Details AMiBA: Array for Microwave Background Anisotropy AMiBA: Array for Microwave Background Anisotropy

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..374u&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 7, p. 374 - 382 (2003)

Astronomy and Astrophysics

Astronomy

1

Interferometers, Arrays, Cosmic Microwave Background

Scientific paper

AMiBA (Array for Microwave Background Anisotropy) is a dual-channel 85-105 GHz interferometric array with full polarization capabilities sited on Mauna-Loa in Hawaii, being built by collaboration between ASIAA/NTU in Taiwan and the Australia Telescope Facility. AMiBA is specifically designed to probe the polarization properties of the Cosmic Microwave Background (CMB) as well as to search for high redshift galaxy clusters via Sunyaev-Zel'dovich effect. Here we review the basic concepts and design details of AMiBA, and explore its potential especially for measuring the CMB temperature and polarization power spectra.

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