Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-03-17
Astrophys.J. 617 (2004) 765-781
Astronomy and Astrophysics
Astrophysics
23 pages, 17 figures, accepted for publication in ApJ
Scientific paper
10.1086/425676
When applied to deep photometric catalogs, the two-point angular correlation function, w(theta), is a sensitive probe of the evolution of galaxy clustering properties. Here we present measurements of w(theta) as a function of I_AB magnitude and (R-I) color to a depth of I_AB=24, using a sample of ~350,000 galaxies covering 5 degrees^2 in total over 5 separate fields. Using redshifts of 3319 galaxies in early DEEP2 Galaxy Redshift Survey data, we construct robust galaxy redshift distributions as a function of I_AB and R_AB magnitude and (R-I) color for galaxies between 0
Coil Alison L.
Davis Martin
Kaiser Nick
Kocevski Dale D.
Koo David C.
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