The Spitzer Deep, Wide-Field Survey (SDWFS)

Details The Spitzer Deep, Wide-Field Survey (SDWFS) The Spitzer Deep, Wide-Field Survey (SDWFS)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21440708a&link_type=abstract

American Astronomical Society, AAS Meeting #214, #407.08; Bulletin of the American Astronomical Society, Vol. 41, p.670

Astronomy and Astrophysics

Astronomy

Scientific paper

The Spitzer Deep, Wide-Field Survey (SDWFS) is four-epoch infrared survey of ten square degrees in the Bootes field of the NOAO Deep Wide-Field Survey using the IRAC instrument on the Spitzer Space Telescope. The four epochs, which span the interval from 2003 to 2008, make it possible to identify nearby, high-proper-motion targets, as well as infrared-variable objects. SDWFS is a Spitzer Cycle 4 Legacy program (PID 40839). The SDWFS catalogs are publicly available, and contain roughly 7e5, 5e5, 1e5, and 1e5 distinct sources brighter than the 5-sigma survey limits of 19.8, 18.8, 16.5, and 15.8 Vega magnitudes at 3.6, 4.5, 5.8, and 8.0 microns, respectively. In this contribution we describe the SDWFS survey and some initial findings.
This work was supported by NASA grant number 1314516, administered by JPL.

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