GEMS: Galaxy Evolution from Morphologies and SEDs

Hans-Walter Rix, Marco Barden, Steven V. W. Beckwith, Eric F. Bell, John A. R. Caldwell, Boris Haeussler, Knud Jahnke, Shardha Jogee, Daniel H. McIntosh, Klaus Meisenheimer, Chien Y. Peng, Sebastian F. Sanchez, Rachel S. Somerville, Lutz Wisotzki, Christian Wolf

Published 2004-01-21Version 1

GEMS, Galaxy Evolution from Morphologies and SEDs, is a large-area (800 arcmin2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on HST. Centered on the Chandra Deep Field South, it covers an area of ~28'x28', or about 120 Hubble Deep Field areas, to a depth of m_AB(F606W)=28.3 (5sigma and m_AB(F850LP)=27.1 (5sigma) for compact sources. In its central ~1/4, GEMS incorporates ACS imaging from the GOODS project. Focusing on the redshift range 0.2<=z<=1.1, GEMS provides morphologies and structural parameters for nearly 10,000 galaxies where redshift estimates, luminosities and SEDs exist from COMBO-17. At the same time, GEMS contains detectable host galaxy images for several hundred faint AGN. This paper provides an overview of the science goals, the experiment design, the data reduction and the science analysis plan for GEMS.