Abstract
We describe the design and performance of Bolocam, a 144-element, bolometric, millimeter-wave camera. Bolocam is currently in its commissioning stage at the Caltech Submillimeter Observatory. We compare the instrument performance measured at the telescope with a detailed sensitivity model, discuss the factors limiting the current sensitivity, and describe our plans for future improvements intended to increase the mapping speed.
Original language | English (US) |
---|---|
Title of host publication | Proceedings of SPIE - The International Society for Optical Engineering |
Editors | T.G. Phillips, J. Zmuidzinas |
Pages | 30-40 |
Number of pages | 11 |
Volume | 4855 |
DOIs | |
State | Published - 2002 |
Externally published | Yes |
Event | Millimeter and Submillimeter Detectors for Astronomy - Waikaloa, HI, United States Duration: Aug 25 2002 → Aug 28 2002 |
Other
Other | Millimeter and Submillimeter Detectors for Astronomy |
---|---|
Country/Territory | United States |
City | Waikaloa, HI |
Period | 8/25/02 → 8/28/02 |
Keywords
- Bolometer arrays
- Bolometers
- Diffraction-limited optics
- Millimeter-wave
ASJC Scopus subject areas
- Electrical and Electronic Engineering
- Condensed Matter Physics