Bolometric properties of OGLE-2014-SN-131 as derived from the BB fit to the SEDs. BB temperature, radius and luminosity are shown by black squares. We only have post-peak SEDs, as before peak OGLE14-131 was only observed in the I band. In the bottom panel we shift the absolute I-band magnitude light curve of OGLE14-131 to match its bolometric light curve after peak. We use the combined bolometric plus shifted I band as the final bolometric light curve, in order to also be able to model its rising part.