[Previous] | [Session 106] | [Next]
A.L. Coil (Univ. California at Berkeley), DEEP2 Team
I will discuss early results from the DEEP2 Redshift Survey on galaxy clustering at z~1 as a function of color, spectral type and luminosity. We find that red, absorption-dominated, passively-evolving galaxies are more strongly clustered than blue, emission-line, actively star-forming galaxies. Intrinsically brighter galaxies also cluster more strongly than fainter galaxies at z~1. We find that the galaxy bias for the DEEP2 sample is ~1.0-1.2. I will also discuss measurements of angular galaxy correlations in our DEEP2 photometric data and the dependence of galaxy clustering on redshift and color, focusing on the evolution of clustering from z~0-1.
[Previous] | [Session 106] | [Next]
Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.