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Fig. 10.


Four systems in which we identify pulsations but where we have doubts about their nature (see Sect. 4.3). The KICs 5217733 and 6806632 could be either SPB or γ Dor/δ Sct. The KIC 6889235, also known as KOI 74, is likely white dwarfs orbiting an A star with tidally excited oscillations. The KIC 7749504 is either a rotational or a Maia variable.

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