This directory contains the bolometric light curves for all the SNeII in the CSP-I sample. We publish bolometric flux LCs instead of luminosities so any future user can choose different distance estimations for their analysis.
Each file contains:

JD: Julian date
fqbol: pseuso-bolometric flux, that is, the integration of the observed fluxes.
ircorr: extrapolated flux from the reddest observed band to infinity.
uvcorr: extrapolated flux from the bluest observed band to zero or 2000A, depending on the method (see Martinez et al. 2021).
fbol: bolometric flux.
