Table 1.
Summary table of the compiled SN sample, along with important properties of the host, namely, its heliocentric redshift (as adopted from the OSC) and reddening caused by the dust in the Milky Way (Schlafly & Finkbeiner 2011).
Host | zhelio | E(B − V)MW | SN | Nspec | Nphot (bands) | References |
---|---|---|---|---|---|---|
M61 | 0.00522 | 0.0193 | 2008in | 6 | 22 (BVRI) | Nakano et al. (2008), de Jaeger et al. (2019) |
2020jfo | 7 | 21 (gri) | Schulze et al. (2020), Sollerman et al. (2021) | |||
NGC 772 | 0.00825 | 0.0623 | 2003hl | 1 | 36 (BVRI) | Moore et al. (2003), Faran et al. (2014) |
2003iq | 4 | 44 (BVRI) | Llapasset et al. (2003), Faran et al. (2014) | |||
NGC 922 | 0.01028 | 0.0163 | 2002gw | 3 | 34 (BVI) | Monard (2002), Galbany et al. (2016) |
2008ho | 2 | 11 (BV) | Pignata et al. (2008); Anderson et al. (in prep.) | |||
NGC 6946 | 0.00013 | 0.2967 | 2004et | 6 | 40 (BVRI) | Zwitter et al. (2004), Faran et al. (2014) |
2017eaw | 8 | 96 (BVRI) | Wiggins (2017), Szalai et al. (2019) |
Notes. References are provided for the discovery and photometry of the objects; for details on the spectroscopy, see Sect. 4.
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