SWIRE: The SIRTF wide-area infrared extragalactic survey

Lonsdale, Carol and Smith, Harding E. and Rowan-Robinson, Michael and Surace, Jason and Shupe, Dave and Xu, Chuanlong and Oliver, Seb and Padgett, Deborah and Fang, Fan and Conrow, Tim and Franceschini, Alberto and Gautier, Nick and Griffin, Mark and Hacking, P. and Masci, Frank and Morrison, Glenn and O'Linger, JoAnne and Owen, Frazer and Perez-Fournon, Ismael and Pierre, Margurite and Puetter, Rick and Stacey, Gordon and Castro, S. and Polletta, Maria and Farrah, Duncan and Jarrett, Tom and Frayer, Dave and Siana, Brian and Babbedge, Tom and Dyer, Steve and Fox, Martin T. and Gonzalez-Solares, Eduardo and Salaman, M. and Berta, Stefano and Condon, J.J. and Dole, Herve and Serjeant, Steve (2003) SWIRE: The SIRTF wide-area infrared extragalactic survey. Publications of the Astronomical Society of the Pacific, 115 (810). pp. 897-927. ISSN 0004-6280. (doi:https://doi.org/10.1086/376850) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided)

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The SIRTF Wide-Area Infrared Extragalactic Survey (SWIRE), the largest SIRTF Legacy program, is a wide-area imaging survey to trace the evolution of dusty, star-forming galaxies, evolved stellar populations, and active galactic nuclei (AGNs) as a function of environment, from redshifts to the current z similar to 3 epoch. SWIRE will survey seven high-latitude fields, totaling 60 - 65 deg(2) in all seven SIRTF bands: Infrared Array Camera (IRAC) 3.6, 4.5, 5.6, and 8 mum and Multiband Imaging Photometer for SIRTF (MIPS) 24, 70, and 160 mum. Extensive modeling suggests that the Legacy Extragalactic Catalog may contain in excess of 2 million IR-selected galaxies, dominated by (1) similar to 150,000 luminous infrared galaxies (LIRGs; L-FIR > 10(11) L-.) detected by MIPS (and significantly more detected by IRAC), similar to 7000 of these with z > 2; (2) 1 million IRAC-detected early-type galaxies (similar to2 x 10(5) with z > 1 and similar to 10,000 with z > 2); and (3) similar to 20,000 classical AGNs detected with MIPS, plus significantly more dust-obscured quasi-stellar objects/AGNs among the LIRGs. SWIRE will provide an unprecedented view of the evolution of galaxies, structure, and AGNs. The key scientific goals of SWIRE are ( 1) to determine the evolution of actively star forming and passively evolving galaxies in order to understand the history of galaxy formation in the context of cosmic structure formation; ( 2) to determine the evolution of the spatial distribution and clustering of evolved galaxies, starbursts, and AGNs in the key redshift range 0.5 < z < 3 over which much of cosmic evolution has occurred; and (3) to determine the evolutionary relationship between "normal galaxies" and AGNs and the contribution of AGN accretion energy versus stellar nucleosynthesis to the cosmic backgrounds. The large area of SWIRE is important to establish statistically significant population samples over enough volume cells that we can resolve the star formation history as a function of epoch and environment, i.e., in the context of structure formation. The large volume is also optimized for finding rare objects. The SWIRE fields are likely to become the next generation of large "cosmic windows" into the extragalactic sky. They have been uniquely selected to minimize Galactic cirrus emission over large scales. The Galaxy Evolution Explorer will observe them as part of its deep 100 deg(2) survey, as will Herschel. SWIRE includes similar to 9 deg(2) of the unique large-area XMM Large Scale Structure hard X-ray imaging survey and is partly covered by the UKIDSS deep J and K survey. An extensive optical/near-IR imaging program is underway from the ground. The SWIRE data are nonproprietary; catalogs and images will be released twice yearly, beginning about 11 months after SIRTF launch. Details of the data products and release schedule are presented.

Item Type: Article
Additional information: 166 UNIV CHICAGO PRESS 704DK
Subjects: Q Science
Divisions: Faculties > Sciences > School of Physical Sciences
Depositing User: Maggie Francis
Date Deposited: 10 Sep 2008 12:27 UTC
Last Modified: 16 Jul 2014 13:46 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/11789 (The current URI for this page, for reference purposes)
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