Fig. C.1.
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Sloan–Pan-STARRS gP1rP1iP1 band light curves of the BL Her-type T2Cep stars analyzed in this work. Horizontal dashed black lines correspond to the determined mean magnitudes. Different colors indicate the different telescopes used during the data collection, while black crosses mark points rejected from the fitting. Black lines show the best-fit Fourier series.
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