The paper Low luminosity Type II supernovae III. SN 2018hwm, a faint event with an unusually long plateau was published in MNRAS, 501, 1059 1071 (2021). After the publication of the paper, we realised that there was an error in the bolometric light curve of SN 2018hwm reported in fig. 7 (top panel), which was one order of magnitude fainter than the luminosity reported correctly in fig. 6 (bottom panel). As a consequence, the average luminosity of the plateau, as shown in fig. 7, is ?3 1040 erg s?1 instead of ?3 1041 erg s?1. The input bolometric light curve used for the modelling was hence 10 times fainter that the correct luminosity, and the SN parameters inferred from the modelling need to be revised.
Áreas temáticas de ASJC Scopus
- Astronomía y astrofísica
- Ciencias planetarias y espacial