arXiv (OAI Expanded)
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Properties of the circumstellar matter around the pair-instability supernova candidate SN 2018ibb revealed by its light curve
SN 2018ibb is one of the best pair-instability supernova (PISN) candidates identified to date. It, however, showed unexpected blue flux excess in late-phase spectra, likely originating from the interaction between supernova (SN) ejecta and dense circumstellar matter (CSM). We develop synthetic light
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