The scale of homogeneity in the Las Campanas Redshift Survey

We analyze the Las Campanas Redshift Survey using the integrated conditiona l density (or density of neighbors) in volume-limited subsamples up to unpr ecedented scales (200 Mpc h(-1)) in order to determine without ambiguity th e behavior of the density field. We find that the survey is well described by a fractal up to 20-30 Mpc h(-1) but flattens toward homogeneity at large r scales. Although the data are still insufficient to establish with high s ignificance the expected homogeneous behavior, and therefore to rule out a fractal trend to larger scales, a fit with a cold dark matter-like spectrum with high normalization well represents the data.