The Spitzer Extragalactic Representative Volume Survey (SERVS)

Details The Spitzer Extragalactic Representative Volume Survey (SERVS) The Spitzer Extragalactic Representative Volume Survey (SERVS)

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944619m&link_type=abstract

American Astronomical Society, AAS Meeting #219, #446.19

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We present details of the Spitzer Extragalactic Representative Volume Survey (SERVS), an 18 square degrees medium-deep survey at 3.6 and 4.5 μm with the post-cryogenic Spitzer Space Telescope to ≈ 2 μJy (AB=23.1) depth of five highly observed astronomical fields (Elais-N1, Elais-S1, Lockman Hole, Chandra-Deep Fied South and XMM). Data will be made available to the community in the Spring of 2012. SERVS is designed to enable the study of galaxy evolution as a function of environment from z ≈ 5 to the present day, and is the first extragalactic survey both large enough and deep enough to put rare objects such as luminous quasars and galaxy clusters at z ≥ 1 into their cosmological context. SERVS is designed to overlap with several key surveys at optical, near- through far-infrared, submillimeter and radio wavelengths to provide a coherent picture of the formation of massive galaxies.

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