Session 54 - Large Scale Structure.
Display session, Tuesday, January 16
North Banquet Hall, Convention Center

## [54.06] The Galaxy-Galaxy Autocorrelation Function for the Las Campanas Redshift Survey

D. L. Tucker, V. Müller, S. Gottlöber (Astrophys. Inst. Potsdam), A. A. Oemler Jr. (Yale, OCIW), R. P. Kirshner (CFA), H. Lin (U. Toronto), S. A. Shectman, S. D. Landy (OCIW), P. L. Schechter (MIT)

The Las Campanas Redshift Survey (LCRS) is a galaxy survey which extends to a redshift of 0.2 and which is composed of a total of 6 alternating 1.5^\circ \times 80^\circ Slices in the North and South Galactic Caps. Now in its final stages, the Survey contains approximately 26,400 galaxy redshifts. We present here a definitive LCRS galaxy-galaxy autocorrelation function \xi_gg(s), its comparison to the \xi_gg(s) from various theoretical models, and a discussion of the impact of the unique character of the LCRS galaxy selection criteria on the measurement of the observed \xi_gg(s).