Fig. 13.

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Impact of the light curve bump between tmax+240 and tmax+340 days on the SN spectrum at tmax+286.7 days. Top: The spectra before, during and after the light curve bump. Bottom: The observed spectrum at tmax+286.7 days (≈13 days before the peak of the bump) is shown in black. We estimate the “bump-free” spectrum of SN 2018ibb at tmax+286.7 days (red) based on the spectra obtained before and after the bump. The difference between the observed (black) and interpolated (red) spectra at tmax+286.7 days is shown in blue. It reveals a series of emission lines that can be attributed to [O II] and [O III]. An excess bluewards of 5000 Å is also visible, while no apparent residual can be seen at the location of [O I].
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