The Galaxy-Absorber Cross-Correlation Function

Abstract

We describe an analysis of the galaxy-absorber cross-correlation function as a function of velocity separation, impact parameter separation, and absorber Lyman alpha equivalent width on impact parameter scales that extend up to 1 Mpc.

6 pages, LaTex, 3 figures, to be published in proceedings of the 13th IAP Meeting, ed. P. Petitjean and S. Charlot