Galaxies, AGN, and Environment at z=1: IRAC observations of DEEP2

Details Galaxies, AGN, and Environment at z=1: IRAC observations of DEEP2 Galaxies, AGN, and Environment at z=1: IRAC observations of DEEP2

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50660j&link_type=abstract

Spitzer Proposal ID #50660

Computer Science

Scientific paper

The Spitzer view of the z=1 Universe is spectroscopy starved. Only 5 sq. deg. of the sky have been surveyed with very deep (24th mag) spectroscopy that probes z>1 galaxies, and only about half of this area has been observed with Spitzer. Cosmic variance is severe even at z>1 and limits our ability to measure the evolution of galaxies and AGN at these epochs. DEEP2 is the premier z>1 wide-field survey, but only 1.5 sq. deg. of it has Spitzer coverage. Here we propose to more than double the overlap between Spitzer and DEEP2, with IRAC coverage of two fields that contain ~16,000 high-quality Keck spectra of galaxies at 0.7

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