Follow-up of Extragalactic SWIRE Sources

Details Follow-up of Extragalactic SWIRE Sources Follow-up of Extragalactic SWIRE Sources

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..136w&link_type=abstract

Spitzer Proposal ID #136

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Scientific paper

We propose to make IRS long-low spectrometer observations of 6 galaxies in the SWIRE Lockman Deep Field (RA = 10h45m; Dec=+59d), selected to be high redshift, extremely luminous IR galaxies (from photo-z) or other unique candidates from optical/IRAC/MIPS/radio color-color relations. For S_24 = 1.0 mJy (10 sigma SWIRE detection) a complete 14-40 micron spectrum may be obtained in 1 hr integration with S/N ~ 5 in the continuum from 13--30 microns, with modest re-binning. From our survey model we expect several hundred IR-bright galaxies to this flux density limit, tens of them with z>2.

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