SWIRE Galactic Follow-up

Details SWIRE Galactic Follow-up SWIRE Galactic Follow-up

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..134w&link_type=abstract

Spitzer Proposal ID #134

Physics

Scientific paper

We intend to perform SIRTF IRS short-low observations of interesting galactic sources discovered by the SWIRE photometric surveys. We expect our targets to fall into one of two categories. The first class is circumstellar debris disks, characterized by an excess of 24 and/or 70 micron emission over photospheric levels in a stellar source. The second is cool brown dwarfs, characterized by a deficit of 3.6 microns to 4.8 microns flux in a faint stellar source.

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