期刊
NEW ASTRONOMY REVIEWS
卷 50, 期 11-12, 页码 993-998出版社
ELSEVIER SCI LTD
DOI: 10.1016/j.newar.2006.09.026
关键词
cosmology; experiment; cosmic microwave background; polarization
资金
- Science and Technology Facilities Council [PP/D00120X/1] Funding Source: researchfish
- STFC [PP/D00120X/1] Funding Source: UKRI
Clover is a new instrument being built to detect the B-mode polarization of the CMB. It consists of three telescopes operating at 97, 150, and 220 GHz and will be sited in Chile at the Llano de Chajnantor. Each telescope assembly is scaled to give a constant beam size of 8 and feeds an array of between 320 and 512 finline-coupled TES bolometers. Here we describe the design, current status and scientific prospects of the instrument. (c) 2006 Elsevier B.V. All rights reserved.
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