  We present the Las Campanas Distant Cluster Survey, which has produced over a
thousand galaxy cluster candidates at 0.35 < z < 1.1 (see Gonzalez et al. 2001
for the full catalog). We discuss the technique that enabled us to use short (~
3 min) exposures and a small (1m) telescope to efficiently survey ~ 130 sq.
deg. of sky. Follow-up imaging and spectroscopy using a wide array of
telescopes including the Keck and VLT suggest that the bona-fide cluster
fraction is ~70%. We construct methods to estimate both the redshift and
cluster mass from the survey data themselves and discuss our first result on
large-scale structure, the dependence of the cluster correlation length with
mean cluster separation at z ~ 0.5 (Gonzalez, Zaritsky, & Wechsler 2001).
