The Spitzer Warm Mission: Hot Science with a "Warm" Telescope

Details The Spitzer Warm Mission: Hot Science with a "Warm" Telescope The Spitzer Warm Mission: Hot Science with a "Warm" Telescope

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dps....39.3403s&link_type=abstract

American Astronomical Society, DPS meeting #39, #34.03; Bulletin of the American Astronomical Society, Vol. 39, p.479

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The Spitzer Space Telescope is the infrared component of NASA's family of Great Observatories comprised of the Chandra X-ray Observatory, the Compton Gamma Ray Observatory, and the Hubble Space Telescope. Cryogenically cooled and in Earth-trailing orbit, Spitzer currently offers imaging capabilities from 3.6-160 microns, and spectroscopy from 5-38 microns.
In approximately March 2009, the liquid helium cryogen on-board Spitzer will be expended, but the observatory will remain operative with 3.6 and 4.5 micron imaging capabilities over two 5'x5’ fields-of-view. Sensitivity in these channels will remain unchanged from the cryogenic mission.
In this "warm” mission phase, Spitzer can operate until early 2014 with high-efficiency, providing up to 35,000 hours of science observing time. This enables several unprecedented opportunities to address fundamental and key scientific questions requiring large allocations of observing time, while maintaining opportunities for broad community use with more "traditional” time allocations.
This poster summarizes some of the possible large scientific programs enabled by a Spitzer warm mission, including support for theory and archival programs. The content is summarized from contributed white papers to the Spitzer Warm Mission workshop, held in Pasadena, CA in June 2007.
For detailed information on these and other science programs possible with warm Spitzer observations, please see: http://ssc.spitzer.caltech.edu/mtgs/warm/

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