SN 2024abfo: A partially stripped type II supernova from a yellow supergiant

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Table A.4.

Properties of the identified or modelled progenitors of SNe IIb. SN 1987A is also added for comparison.

Object	Progenitor	log(T_eff/K)	log(L/L_⊙)	Radius	Mass	SN has	Peak abs.	Reference
	detected			(R_⊙)	(M_⊙)	1st peak?	Mag (r/R)
SN 1987A	Yes (BSG)	4.20±0.04	5.04±0.10	45±15	∼20	-	−16.4	Podsiadlowski (1992)

SN 1993J	Yes (RSG)	3.63±0.05	5.1±0.3	600	15	Yes	−17.6	Maund et al. (2004)
SN 2008ax	Yes (BSG)	4.05 $_{- 0.17}^{+ 0.25}$ $^{+0.25}_{-0.17}$	4.69 $_{- 0.27}^{+ 0.61}$ $^{+0.61}_{-0.27}$	50	< 25	No	−18.0	Folatelli et al. (2015)
SN 2011dh	Yes (YSG)	3.78±0.02	4.92±0.20	200	13±3	No?	−17.2	Maund et al. (2011)
SN 2011fu	No	-	-	450	13-18	Yes	−18.1	Morales-Garoffolo et al. (2015)
SN 2011hs	No	-	-	500-600	12-15	No	−16.9	Bufano et al. (2014)
SN 2013df	Yes (RSG)	3.63±0.01	4.94±0.06	600	13-17	Yes	−17.8	Van Dyk et al. (2014)
SN 2016gkg	Yes (BSG)	3.98 $_{- 0.16}^{+ 0.21}$ $^{+0.21}_{-0.16}$	5.14 $_{- 0.39}^{+ 0.22}$ $^{+0.22}_{-0.39}$	140 $_{- 100}^{+ 130}$ $^{+130}_{-100}$	15-20	Yes	−17.2	Kilpatrick et al. (2017)
SN 2017gkk	Yes (YSG)	3.72±0.08	5.17±0.04	-	16	-	-	Niu et al. (2024)
SN 2024abfo	Yes (YSG)	3.80-3.85	5.00±0.05	215-270	15	faint	−16.5	This work

Notes. If the progenitor was not detected in archival images its parameters are inferred from hydrodynamical modelling. The masses reported are the initial masses of the progenitors. We note that an early peak might be visible in the g-band light curve of SN 2011dh published by Arcavi et al. (2011).

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