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SWIRE and SIRTF Surveys

Published online by Cambridge University Press:  23 September 2016

Carol J. Lonsdale
Carol J. Lonsdale*
Affiliation:
Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA

Abstract

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The launch of SIRTF on August 25, 2003 opens an exciting new era for the infrared. Building on the legacy of IRAS, COBE & ISO, SIRTF will image the sky from 3.6–160 μm in tiered surveys, from wide (∼80 sq. deg.) reaching z∼1 in depth for L*FIR galaxies, to small, deep, confusion-limited surveys. SIRTF will measure the accumulation of stellar mass at high redshift, and the evolution of dusty systems (disks, starbursts & AGN) since z∼4, on size scales up to several hundred Mpc. The next decade will also see two major all-sky IR surveys, ASTRO-F and WISE (Wide-field Infrared Survey Explorer), and the launch of Herschel and Planck.

Type
Session VI: The Distant Universe
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 337 - 346
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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