Fig. B.1.
K-corrections in the r-band for SNe IIn at different redshifts. Blue points are the corrections computed for well-studied SNe IIn available in the literature (see the text for more details). Green lines are the best-fit models obtained using third-order polynomials, while dashed lines are the 1σ uncertainties of each fit. Phases (rest frame) refer to the estimated light-curve peak (Sect. 4.1 and Table 6) of each SN in the sample.
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