  We describe the status of a project whose main goal is to detect variability
along the extreme horizontal branch of the globular cluster NGC 6752. Based on
Magellan 6.5m data, preliminary light curves are presented for some candidate
variables. By combining our time-series data, we also produce a deep CMD of
unprecedented quality for the cluster which reveals a remarkable lack of main
sequence binaries, possibly pointing to a low primordial binary fraction.
