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

https://doi.org/10.26131/IRSA324
https://www.ipac.caltech.edu/doi/10.26131/IRSA324

10.26131/IRSA324

IPAC

SWIRE team

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

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.

The SWIRE Lockman Hole ISOCAM Deep Field Catalog presents MIPS 24 micron measurements of the sources detected at 14.3 micron in the Lockman Hole Shallow Survey by ISO. For more details on the Lockman Hole ISOCAM Shallow Survey, see Fadda et al. (2004).

This dataset or service is made available by the Infrared Science Archive (IRSA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Dataset

https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=swire_lhisos