Dark Energy: Measurement by the DEEP2 Redshift Survey

Details Dark Energy: Measurement by the DEEP2 Redshift Survey Dark Energy: Measurement by the DEEP2 Redshift Survey

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..apr.u3001d&link_type=abstract

American Physical Society, APS April Meeting, April 16-19, 2005, abstract #U3.001

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The DEEP2 redshift survey has now covered ˜2.5 degrees^2 of sky and obtained nearly 40,000 spectra; the survey is nearly finished, and I shall describe what has been accomplished with all that Keck time! One of our fields is the Extended Groth Strip (EGS), a region where deep imaging is being obtained with Chandra, Spitzer, GALEX, VLA, and HST/ACS and will be the subject of Sunyaev-Zel'dovich observations. We will eventually provide 17,000 redshifts. In three other regions, we have used three-color imaging to efficiently select galaxies with magnitude RAB<24.1 and redshifts in the range 0.7

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