2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/11555We 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. CharlotAstrophysicstext