Fig. B.4.
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ZTF light curves of four known candidate magnetic period bouncers with a low accretion rate (Breedt et al. 2012 and Kawka et al. 2021; see Schreiber et al. 2023 for an overview). These systems only show very subtle (few percent amplitude) periodic variability that is also visible in ZTF data but not enough to identify these objects as magnetic period bouncers.
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