The Galaxy-Absorber Cross-Correlation Function
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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
6 pages, LaTex, 3 figures, to be published in proceedings of the 13th IAP Meeting, ed. P. Petitjean and S. Charlot