Table 1.
Confirmed and likely CCSNe at the central regions (dproj ≤ 2.5 kpc) of LIRGs with SED model based global star formation properties of LIRG hosts (see compilations of Kool et al. 2018; Kool 2019, and references therein).
Host | Dl | log(LIR) | tSB | SNRSB | SFR | LAGN | SED | DOF | CCSN | Type | dproj |
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Disc. | Ref. |
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(Mpc) | (L⊙) | (Myr) | (SN yr−1) | (M⊙ yr−1) | (%) | host | (kpc) | (mag) | ||||||
IRAS 18293−3413 | 84.1 | 11.89 |
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S | 22 | AT 2012iz | IIP | 0.6 | 1.8 | IR | (1) |
IRAS 18293−3413 | … | … | … | … | … | … | … | … | SN 2013if | IIP | 0.2 | 0 | IR | (2) |
IC 883 | 107.1 | 11.73 |
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D | 27 | SN 2010cu | IIP | 0.2 | 0 | IR | (3) |
IC 883 | … | … | … | … | … | … | … | … | SN 2011hi | IIP | 0.4 | 6 | IR | (3) |
NGC 5331 | 150.0 | 11.66 |
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D | 5 | AT 2017chi | IIn | 1.5 | 12 | IR | (1) |
Arp 299 | 44.8 | 11.82 |
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0.0 | S | 5 | SN 1998T | Ib | 1.5 | ? | Opt | (4) |
Arp 299 | … | … | … | … | … | … | … | … | SN 2005U | IIb | 1.4 | ? | IR | (4) |
Arp 299 | … | … | … | … | … | … | … | … | SN 2010O | Ib | 1.2 | 1.9 | Opt | (5) |
Arp 299 | … | … | … | … | … | … | … | … | SN 2010P | IIb | 0.2 | 7 | IR | (5) |
Arp 299 | … | … | … | … | … | … | … | … | SN 2019lqo | IIb | 2.0 | 2.1 | Opt | (6) |
Arp 299 | … | … | … | … | … | … | … | … | SN 2020fkb | Ib | 0.7 | 0.4 | Opt | (6) |
NGC 1614 | 66.8 | 11.66 |
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S | 33 | SN 1996D | Ic | 2.1 | ? | Opt | (2) |
NGC 1614 | … | … | … | … | … | … | … | … | SN 2020cuj | II | 2.5 | 2.8 | Opt | (5) |
NGC 838 | 53.3 | 11.05 |
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S | 7 | SN 2005H | II | 0.4 | ? | Opt | (2) |
IRAS 17138−1017 | 82.2 | 11.49 |
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S | 22 | SN 2008cs | IIn | 1.5 | 16 | IR | (7) |
IRAS 17138−1017 | … | … | … | … | … | … | … | … | SN 2015cb | IIP | 0.6 | 4.6 | IR | (2) |
NGC 2388 | 61.1 | 11.28 |
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D | 8 | SN 2015U | Ibn | 1.8 | 3.1 | Opt | (8) |
NGC 317B | 77.0 | 11.19 |
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S | 30 | SN 1999gl | II | 1.9 | ? | Opt | (2) |
NGC 317B | … | … | … | … | … | … | … | … | SN 2014dj | Ic | 1.5 | ? | Opt | (2) |
NGC 3256 | 37.4 | 11.61 |
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S | 16 | SN 2001db | II | 2.1 | 5.5 | IR | (6) |
NGC 3256 | … | … | … | … | … | … | … | … | PSN102750 | IIn | 2.1 | 0.3 | Opt | (6) |
NGC 3256 | … | … | … | … | … | … | … | … | SN 2018ec | Ic | 1.7 | 2.1 | IR | (6) |
NGC 3256 | … | … | … | … | … | … | … | … | AT 2018cux | IIP | 0.8 | 2.1 | Opt | (6) |
ESO 138−G27 | 96.1 | 11.41 |
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S | 27 | SN 2009ap | Ic | 1.2 | ? | Opt | (2) |
NGC 6907 | 49.2 | 11.11 |
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S | 2 | SN 2008fq | II | 1.4 | ? | Opt | (2) |
NGC 2146 | 18.0 | 11.15 |
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S | 8 | SN 2005V | Ib/c | 0.5 | ? | IR | (2) |
MCG -02-01-052 | 115.2 | 11.48 |
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S | 3 | SN 2010hp | II | 2.1 | 0.5 | IR | (9) |
NGC 6000 | 28.1 | 10.95 |
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S | 4 | SN 2010as | IIb | 0.6 | 1.8 | Opt | (10) |
NGC 5433 | 70.3 | 11.01 |
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< 0.03 |
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S | 2 | SN 2010gk | Ic | 2.0 | ? | Opt | (2) |
Notes. Luminosity distances are obtained via NED. References for the CCSNe and their host galaxy extinction estimates, if available, are given in brackets.
References. 1) Kool (2019), 2) Kool et al. (2018), 3) Kankare et al. (2012), 4) Mattila et al. (2012), 5) Kankare et al. (2014a), 6) This work, 7) Kankare et al. (2008), 8) Pastorello et al. (2015), 9) Miluzio et al. (2013), 10) Folatelli et al. (2014).
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