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Proceedings Paper

FORCAST: the facility mid-IR camera for SOFIA
Author(s): Joseph D. Adams; Terry L. Herter; Luke D. Keller; George E. Gull; Bruce Pirger; Justin Schoenwald; Marc Berthoud; Gordon J. Stacy; Thomas Nikola
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Paper Abstract

We report on new development and testing of FORCAST, the Faint Object infraRed Camera for the SOFIA Telescope. FORCAST will offer dual channel imaging in discrete filters at 5 - 25 microns and 30 - 40 microns, with diffraction-limited imaging at wavelengths > 15 microns. FORCAST will have a plate scale of 0.75 arcsec per pixel, giving it a 3.2 arcmin x 3.2 arcmin FOV on SOFIA. In addition, a set of grisms will enable FORCAST to perform long slit and cross-dispersed spectroscopic observations at low to moderate resolution (R ~ 140 - 1200) in the bandpasses 4.9 - 8.1 microns, 8.0 - 13.3 microns, 17.1 - 28.1 microns, and 28.6 - 37.4 microns. FORCAST has seen first light at the Palomar 200 inch telescope. It will be available for astronomical observations and facility testing at SOFIA first flight.

Paper Details

Date Published: 28 June 2006
PDF: 11 pages
Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 626911 (28 June 2006); doi: 10.1117/12.671414
Show Author Affiliations
Joseph D. Adams, Cornell Univ. (United States)
Terry L. Herter, Cornell Univ. (United States)
Luke D. Keller, Ithaca College (United States)
George E. Gull, Cornell Univ. (United States)
Bruce Pirger, Cornell Univ. (United States)
Justin Schoenwald, Cornell Univ. (United States)
Marc Berthoud, Cornell Univ. (United States)
Gordon J. Stacy, Cornell Univ. (United States)
Thomas Nikola, Cornell Univ. (United States)


Published in SPIE Proceedings Vol. 6269:
Ground-based and Airborne Instrumentation for Astronomy
Ian S. McLean; Masanori Iye, Editor(s)

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