The SIRTF Wide-area InfraRed Extragalactic (SWIRE) Survey

Details The SIRTF Wide-area InfraRed Extragalactic (SWIRE) Survey The SIRTF Wide-area InfraRed Extragalactic (SWIRE) Survey

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.9009s&link_type=abstract

American Astronomical Society Meeting 203, #90.09; Bulletin of the American Astronomical Society, Vol. 35, p.1351

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Scientific paper

SWIRE, the largest SIRTF Legacy program, is a wide-area imaging survey covering 65 square degrees in 7 high-latitude fields. It's objective is to trace the evolution of dusty, star-forming galaxies (MIPS), evolved stellar populations (IRAC),and active galactic nuclei as a function of environment (ie. spatial distribution/clustering) from 0.5 < z < 2.5. Ancillary data from many other wavelengths has been taken to compliment the infrared, including the deepest VLA image ever taken, the largest wide-area Chandra X-ray survey, and over 100 nights of optical/near-IR imaging to date. The details of these multiwavelength undertakings and their substantial scientific potential will be summarized including preliminary results from the optical/near-IR catalogues and photometric redshifts. This work is supported by NASA-SIRTF Legacy Program Funding to IPAC/UCSD.

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