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Fig. 6.
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TESS light curves, their periodograms, and the light curves phased with the best found period, of five of the targets in which we detected photometric variability. (a) V* V1208 Sco, (b) CPD–41 7717, (c) HD 152200, (d) CXOU J165421.3-415536, (e) CPD–41 7746.
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