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

A Search for EHB Pulsators in the Globular Cluster NGC 6752