Table 6
Fundamental data of observed SN II progenitors with metallicity around solar (log (O/H) + 12 ≃ 8.4−8.7).
SN | d | AV | MR | MI | M555 | M606 | M814 | MJ | MKs | Mini lit. | Refs. | Mini non-rot. | Mini rot. | |
(Mpc) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (M⊙) | (M⊙) | (M⊙) | |||
|
||||||||||||||
1999br | 14.1± 2.6 | 0.06 ± 0.06 | − | − | − | >−5.88 | − | − | − | <15 | MS05, S09b | <14 | <12 | |
1999em | 11.7 ± 1.0 | 0.31 ± 0.16 | − | >−7.49 | − | − | − | − | − | <15 | S09b | <13 | <11 | |
1999gi | 10.0 ± 0.8 | 0.65 ± 0.16 | − | − | − | >−5.67 | − | − | − | <14 | S01, S09b | <13 | <11 | |
2001du | 18.3 ± 1.2 | 0.53 ± 0.28 | − | − | − | − | >−7.36 | − | − | <15 | vD03, S03, S09b | <12 | <10 | |
2002hh | 5.9 ± 0.4 | 5.2 ± 0.2 | − | >−8.15 | − | − | − | − | − | <18 | S09b | <17 | <14 | |
2003gd | 9.3 ± 1.8 | 0.43 ± 0.19 | − | −6.92 ± 0.47 | − | −5.16 ± 0.44 | − | − | − | 8.4 ± 2.0 | S09b, M13 | 10.8 ± 2.1 | 8.5 ± 1.8 | |
2003ie | 15.5 ± 1.2 | 0.04 | >−8.33 | − | − | − | − | − | − | <25 | S09b | <23 | <20 | |
2004dg | 20.0 ± 2.6 | 0.74 ± 0.09 | − | − | − | − | >−6.93 | − | − | <12 | S09b | <10 | <8 | |
2005cs | 8.4 ± 1.0 | 0.43 ± 0.06 | − | − | − | − | −6.75 ± 0.26 | − | − |
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M05, L06, E07, S09b | 8.6 ± 5.4 | 7.5 ± 1.5 | |
2006bc | 14.7 ± 2.6 | 0.64 | − | − | − | − | >−6.75 | − | − | <12 | S09b | <8.5 | <7.5 | |
2006my | 22.3 ± 2.6 | 0.08 | − | − | − | − | −7.37 ± 0.25 | − | − | 9.8 ± 1.7 | M13 | 12.4 ± 3.5 | 10.5 ± 1.5 | |
2007aa | 20.5 ± 2.6 | 0.09 | − | − | − | − | >−7.16 | − | − | <12 | S09b | <11 | <9.5 | |
2009md | 21.3 ± 2.1 | 0.31 | − | − | − | −5.00 ± 0.35 | −6.84 ± 0.33 | − | − |
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F11 | 10.0 ± 1.8 | 8.1 ± 1.4 | |
2009hd | 9.4 ± 0.4 | 3.8 ± 0.14 | − | − | − | − | >8.54 | − | − | <20 | E11 | <20 | <17 | |
2012aw | 10.0 ± 0.4 | 3.1 | − | − | −6.69 ± 0.15 | − | −8.39 ± 0.11 | −9.85 ± 0.10 | −10.88 ± 0.21 | 17−18 | vD12 | 18.9 ± 1.8 | 15.6 ± 0.9 | |
... | ... | ... | − | − | −6.48 ± 0.15 | − | −8.39 ± 0.11 | −9.77 ± 0.22 | −11.2 ± 0.4 | 14−26 | F12 | 18.3 ± 1.8 | 15.5 ± 0.9 |
Notes. All progenitors are from SN IIP, with the exception of the progenitor of SN 2009hd, which was a SN IIL. We quote the distance, reddening, absolute magnitudes in R,I, F555W, F606W, F814W, J, and KS filters, and initial progenitor mass found in the literature, together with our determination of the progenitor’s initial mass based on our rotating and non-rotating models.
Reference. S01 = Smartt et al. (2001); S03 = Smartt et al. (2003); vD03 = Van Dyk et al. (2003); M05 = Maund et al. (2005a); MS05 = Maund & Smartt (2005); L06 = Li et al. (2006); L07 = Li et al. (2007); E07 = Eldridge et al. (2007); S09b = Smartt et al. (2009); E11 = Elias-Rosa et al. (2011); F11 = Fraser et al. (2011); F12 = Fraser et al. (2012); vD12 = Van Dyk et al. (2012); M13 = Maund et al. (2013).
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