期刊
APPLIED OPTICS
卷 46, 期 17, 页码 3444-3454出版社
OPTICAL SOC AMER
DOI: 10.1364/AO.46.003444
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资金
- Direct For Mathematical & Physical Scien
- Division Of Physics [0855887] Funding Source: National Science Foundation
- STFC [PP/D001048/1] Funding Source: UKRI
The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background simultaneously at 145, 215, and 280 GHz with arcminute resolution. Each frequency will have a 32 by 32 element focal plane array of transition edge sensor bolometers. The telescope and the cold reimaging optics are optimized for millimeter-wave observations with these sensitive detectors. The design of each is described. (C) 2007 Optical Society of America.
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