Table A.3
Shift in zero points of the 4 SCM calibrations as a result of fixing the SN distance to the respective Cepheid distance to the host galaxy.
| SN | Δμ (Hamuy 2003b)† | Δμ (Nugent et al. 2006) | Δμ (Poznanski et al. 2009) | Δμ (D’Andrea et al. 2010) |
| (mag) | (mag) | (mag) | (mag) | |
|
|
||||
| 2004dj | 0.24 | 0.33 | 0.22 | 0.43 |
| 2008bk | 0.02 | 0.05 | −0.05 | 0.22 |
| 2014bc | −0.10 | −0.19 | 0.02 | 0.38 |
| 2012aw | −0.14 | 0.07 | −0.37 | −0.21 |
| 1999em | −0.27 | −0.17 | −0.34 | −0.16 |
| 2001du | −0.19 | 0.07 | −0.18 | −0.01 |
Notes. The SNe are ordered in terms of increasing distance. Δμ is given in the sense (SCM−Cepheid).
Hamuy (2003b) Eq. (4). The shifts for SN 2014bc if using the maser distance value are given in Table 1.
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