Fig. 7.
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Wesenheit K corrections for an X Cyg-like Cepheid (16.4 d) at 23 Mpc as a function of phase (by proxy of Teff) and assuming different amounts of host reddening. The most significant phase variation is seen for the highest amount of reddening, where Kext(WH, VI) may differ by as much as 0.01 mag among phases of extreme Teff values.
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