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Fig. E.5
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Same details as in Fig. E.1, but for EPIC 238194885, based on the frequencies used (8.7 and 13.7 μHz) attributed to prograde sectoral modes with m = 1. For this star, the results are: vrot = 7.0 ± 0.3 μHz, P0 = 6.4 ± 0.5 · 103 s.
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