Optical design of the atacama cosmology telescope and the millimeter bolometric array camera
- J. W., Fowler
- M. D., Niemack
- S. R., Dicker
- A. M., Aboobaker
- P. A. R., Ade
- BATTISTELLI, Elia Stefano
- M. J., Devlin
- R. P., Fisher
- M., Halpern
- P. C., Hargrave
- A. D., Hincks
- M., Kaul
- J., Klein
- J. M., Lau
- M., Limon
- T. A., Marriage
- P. D., Mauskopf
- L., Page
- S. T., Staggs
- D. S., Swetz
- E. R., Switzer
- R. J., Thornton
- C. E., Tucker
DOIAbstract
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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