First Look Survey - Galactic Component

Details First Look Survey - Galactic Component First Look Survey - Galactic Component

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003sptz.prop..104s&link_type=abstract

Spitzer Proposal ID #104

Computer Science

Scientific paper

The galactic component of the SIRTF First Look Survey is intended to characterize diffuse emission and point source confusion at a variety of galactic latitudes and in a typical molecular cloud. The strategy involves sparse mapping in 15 arcmin x 1 degree strips with MIPS and IRAC along galactic longitudes 105.6 (galactic latitudes -1.3,0.35, 2.0,4.0,8.0,16.0, and 32.0 degrees) and 254.4 degrees (galactic latitudes 0.0,-2.0,-5.0,-9.0, and -14.0 degrees). In addition, four small IRAC maps at galactic longitude 97.5 (galactic latitudes 0,-4,+4, and +16) will be made to best sample the stellar density of the Galactic disk. The L1228 molecular cloud will be mapped with a 10 arcmin x 2 degree strip with MIPS and IRAC.

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