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J. Newman (Hubble Fellow, Lawrence Berkeley National Laboratory), DEEP2 Team
The DEEP2 Redshift Survey, a three-year project to obtain spectra of > 50,000 galaxies at z>0.7 with the new DEIMOS spectrograph at the Keck Observatory, is more than one-third complete. We now have sufficient data to assess the effects of our color-based redshift preselection and to predict the general characteristics of the final DEEP2 dataset. In this talk, I will summarize the nature of the survey sample and describe the principal selection effects to be aware of. This talk will provide some basic background information for other DEEP2 talks.
The author(s) of this abstract have provided an email address for comments about the abstract: janewman.at.lbl.gov
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.