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Fig. 4.

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Fraction of the IR correction over the bolometric flux as a function of time. The black solid line indicates the mean values within each time bin, while the dashed lines represent the standard deviation. We only include SNe II with observed YJH photometry. Three SNe II (SNe 2005lw, 2007sq and 2009ao) display unusual values beyond 2σ from the mean. This may be due to a significant uncorrected reddening in the host galaxy (see text).

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