Spitzer Wide-area InfraRed Extragalactic Survey Lockman Hole ISOCAM Deep Field MIPS 24 micron Catalog

Description

The Spitzer Wide-area InfraRed Extragalactic survey (SWIRE), the largest Spitzer Legacy program, is a wide-area, imaging survey to trace the evolution of dusty, star-forming galaxies, evolved stellar populations, and AGN as a function of environment, from redshifts z~3 to the current epoch. SWIRE surveys 6 high-latitude fields, totaling ~50 sq. deg. in all 7 Spitzer bands: 3.6, 4.5, 5.8, and 8 microns with IRAC and 24, 70, and 160 microns with MIPS (Lonsdale et al. 2003). The SWIRE Legacy Extragalactic Source Catalogs will eventually contain in excess of 2 million IR-selected galaxies, from those dominated by the light of stellar populations detected primarily by IRAC, to starbursts, ultra-luminous infrared galaxies and AGN detected also by MIPS.\n\nThe SWIRE Lockman Hole ISOCAM Deep Field Catalog presents MIPS 24 micron measurements of the sources detected at 14.3 micron in the Lockman Hole Deep Survey by ISO. For more details on the Lockman Hole ISOCAM Deep Survey, see Rodighiero et al. (2004).

Resources

Name Format Description Link
5 https://irsa.ipac.caltech.edu%2Fdata%2FSPITZER%2FSWIRE%2Fdocs%2Fswire_lh_isocam_deep_colDescriptions.html
5 https://irsa.ipac.caltech.edu%2FSCS%3Ftable%3Dswire_lhisod%26
5 https://irsa.ipac.caltech.edu/SCS?table=swire_lhisod&
21 swire_lh_isocam_deep_colDescriptions.html https://irsa.ipac.caltech.edu/data/SPITZER/SWIRE/docs/swire_lh_isocam_deep_colDescriptions.html

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