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Fig. 1

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The photometric V and K light curves, and the (V − K) colour curve as used in our IRSB analysis for the LMC Cepheid variable HV2282. This is a typical set of photometric light and colour curves in the present study based on the optical photometry from OGLE-III (Udalski et al. 2008; Soszyński et al. 2008), and the near-IR photometry from Persson et al. (2004).

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