Abstract
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.
Original language | English (US) |
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Pages (from-to) | 3444-3454 |
Number of pages | 11 |
Journal | Applied Optics |
Volume | 46 |
Issue number | 17 |
DOIs | |
State | Published - Jun 10 2007 |
All Science Journal Classification (ASJC) codes
- Engineering (miscellaneous)
- Atomic and Molecular Physics, and Optics
- Electrical and Electronic Engineering