Share Email Print

Proceedings Paper

Instrumentation for the CCAT Telescope
Author(s): G. J. Stacey; S. R. Golwala; C. M. Bradford; C. D. Dowell; G. Cortes-Medellin; T. Nikola; J. Zmuidzinas; T. L. Herter; S. J. Radford; J. P. Lloyd; A. W. Blain; R. L. Brown; D. B. Campbell; R. Giovanelli; P. Goldsmith; P. M. Harvey; C. Henderson; W. D. Langer; T. G. Phillips; A. C. S. Readhead; D. P. Woody
Format Member Price Non-Member Price
PDF $17.00 $21.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama Telescope (CCAT). The primary science for CCAT can be achieved through wide field photometric imaging in the short submillimeter through millimeter (200 μm to 2 mm) telluric windows. We present strawman designs for two cameras: a 32,000 pixel short submillimeter (200 to 650 μm) camera using transition edge sensed bare bolometer arrays that Nyquist samples (@ 350 μm) a 5'×5' field of view (FoV), and a 45,000 pixel long wavelength camera (850 μm to 2 mm) that uses slot dipole antennae coupled bolometer arrays with wavelength dependent sampling that covers up to a 20' square FoV. These are our first light instruments. We also anticipate "borrowed" instruments such as direct detection and heterodyne detection spectrometers will be available at, or nearly at first light.

Paper Details

Date Published: 6 July 2006
PDF: 12 pages
Proc. SPIE 6275, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III, 62751G (6 July 2006); doi: 10.1117/12.672176
Show Author Affiliations
G. J. Stacey, Cornell Univ. (United States)
S. R. Golwala, California Institute of Technology (United States)
C. M. Bradford, Jet Propulsion Lab. (United States)
C. D. Dowell, Jet Propulsion Lab. (United States)
G. Cortes-Medellin, Cornell Univ. (United States)
T. Nikola, Cornell Univ. (United States)
J. Zmuidzinas, California Institute of Technology (United States)
T. L. Herter, Cornell Univ. (United States)
S. J. Radford, California Institute of Technology (United States)
J. P. Lloyd, Cornell Univ. (United States)
A. W. Blain, California Institute of Technology (United States)
R. L. Brown, Cornell Univ. (United States)
D. B. Campbell, Cornell Univ. (United States)
R. Giovanelli, Cornell Univ. (United States)
P. Goldsmith, Jet Propulsion Lab. (United States)
P. M. Harvey, Univ. of Texas, Austin (United States)
C. Henderson, Cornell Univ. (United States)
W. D. Langer, Jet Propulsion Lab. (United States)
T. G. Phillips, California Institute of Technology (United States)
A. C. S. Readhead, California Institute of Technology (United States)
D. P. Woody, California Institute of Technology Owens Valley Radio Observatory (United States)

Published in SPIE Proceedings Vol. 6275:
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
Jonas Zmuidzinas; Wayne S. Holland; Stafford Withington; William D. Duncan, Editor(s)

© SPIE. Terms of Use
Back to Top