Strawman Design of a Long-wavelength Camera for the Cornell-Caltech Atacama Telescope

Details Strawman Design of a Long-wavelength Camera for the Cornell-Caltech Atacama Telescope Strawman Design of a Long-wavelength Camera for the Cornell-Caltech Atacama Telescope

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110103g&link_type=abstract

American Astronomical Society, AAS Meeting #211, #101.03; Bulletin of the American Astronomical Society, Vol. 39, p.917

Astronomy and Astrophysics

Astronomy

Scientific paper

The initial suite of instruments for the Cornell Caltech Atacama Telescope (CCAT) will likely include a wide-field, long-wavelength continuum camera (LWCam), covering frequencies from 150 GHz to 405 GHz (740 um to 2 mm) over a field-of view (FoV) as large as 20' diameter. Such a camera would contribute to many of CCAT's science goals and make use of time when poor weather renders short-wavelength (200-600 um) observations unfeasible. A strawman design for such a camera is presented here, including an assessment of the current status of various necessary technologies.

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