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We have identified a star in the Wide Angle Search for Planets (WASP) archive photometry with an unusual light curve due to the total eclipse of a small, hot star by an apparently normal A‐type star and with an orbital period of only 0.668 d. From an analysis of the WASP light curve together with V‐band and IC‐band photometry of the eclipse and a spectroscopic orbit for the A‐type star we estimate...
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