Table 3.
Summary table of the EPM results.
| Host | SN | D [Mpc] | t0 (MJD) | E(B − V) [mag] |
|---|---|---|---|---|
| M61 | 2008in | 15.06(0.71) | 54824.15(0.15) | 0.06(0.03) |
| 2020jfo | 14.95(0.78) | 58975.08(0.34) | 0.07(0.04) | |
| NGC 722 | 2003hl | 33.95(4.49) | 52864.26(1.20) | 0.31( * ) |
| 2003iq | 26.02(1.85) | 52919.20(0.54) | 0.15(0.05) | |
| NGC 922 | 2002gw | 43.46(3.67) | 52555.84(1.15) | 0.12(0.03) |
| 2008ho | 40.02(5.07) | 54789.17(2.12) | 0.21( * ) | |
| NGC 6946 | 2004et | 5.99(0.36) | 53270.62(0.16) | 0.38(0.10) |
| 2017eaw | 6.44(0.29) | 57885.52(0.22) | 0.35(0.04) | |
Notes. t0 denotes the time of explosion as obtained by the EPM regression. The E(B − V) values listed here are those determined by the spectral fitting. The values in brackets denote the uncertainties of the given quantities. In the starred (*) cases we either had only one spectrum to fit or both spectra yielded the same reddening value, which did not allow us to give a reasonable empirical uncertainty.
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