Spitzer Matching Survey of the Ultra-VISTA Deep Stripes

https://doi.org/10.26131/IRSA401
https://www.ipac.caltech.edu/doi/10.26131/IRSA401

10.26131/IRSA401

IPAC

Ashby, M. L. N.; Caputi, Karina I.; Cowley, Will; Deshmukh, Smaran; Dunlop, James S.; Milvang-Jensen, Bo; Fynbo, Johan P. U.; Muzzin, Adam; McCracken, H. J.; Le Fèvre, Olivier; Huang, Jia-Sheng; Zhang, J.

Spitzer Matching Survey of the Ultra-VISTA Deep Stripes

The Spitzer Matching Survey of the Ultra-VISTA Deep Stripes (SMUVS) consists of deep 3.6 and 4.5 imaging of three Ultra-VISTA near-infrared survey stripes in the COSMOS field. SMUVS reaches point-source sensitivities of about 25.0 AB mag at both 3.6 and 4.5 microns with a significance of 4 sigma, accounting for both survey sensitivity and source confusion. To this limit, the SMUVS catalogs contain a total of ~350,000 sources, each of which is detected significantly in at least one IRAC band. Because of its uniform and high sensitivity, relatively large area coverage, and the wide array of ancillary data available in COSMOS, the SMUVS survey will be useful for a large number of cosmological investigations.

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/data/SPITZER/SMUVS