Fig. 2.
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Period–Wesenheit relation in the Gaia bands for the 11 ACEP_Fs (filled green circles) and one ACEP_1O (filled black circle, log P shifted by −0.01 to avoid overlap with F pulsators) in comparison with analoguous data for the LMC (red and blue dots represent ACEP_Fs and ACEP_1Os, respectively). To obtain the absolute Wesenheit magnitude for the LMC stars, we adopted the distance modulus by Pietrzyński et al. (2019).
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