TESS microscope reveals: EA-SD TU Her has not just unusually deep nice primary eclipses, but also fast oscillatons with amplitude about 0.01m and period about 1 hour, which overlaps on the secondary eclipses.
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What I might suggest is take the data while the system is out of eclipse and run a Fourier. The frequency content would give you a good idea if it was a low amplitude delta Scuti.
Eric
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