Fig. 11
Contribution of the UV, optical, and IR fluxes to the bolometric flux of 20 CSP-I SE SNe with at least one epoch of observations spanning from u to H band. The optical flux dominates at all epochs, the NIR flux becomes important at late time, whereas the UV fraction is non-negligible only before maximum. SNe IIb, Ib, Ic, and Ic-BL are represented in green, blue, red, and magenta, respectively.
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