Table A.2
Details of recent type IIP SNe in host galaxies with Cepheid distance measurements.
| SN | Galaxy | v hel * | D Cepheid | E(B − V) | m V 50 | m I 50 | v 50 ** | References |
| (km s-1) | (Mpc) | (mag) | (mag) | (mag) | (km s-1) | |||
|
|
||||||||
| 2004dj | NGC 2403 | 133 | 3.22 (0.15) | 0.100 | 12.04 (0.03) | 11.40 (0.03) | 3250 (250) | 1, 2, 3 |
| 2008bk | NGC 7793 | 230 | 3.44 (0.15) | 0.021 | 12.85 (0.10) | 12.10 (0.10) | 2200 (200) | 4, 5, 6 |
| 2014bc | NGC 4258 | 448 | 7.40 (1.16) | 0.014 | 15.32 (0.10) | 14.60 (0.12) | 1460 (100) | 7 |
| 2012aw | NGC 3351 | 778 | 10.00 (0.41) | 0.086 | 13.54 (0.02) | 12.82 (0.05) | 4250 (200) | 1, 8, 9 |
| 1999em | NGC 1637 | 717 | 11.70 (1.00) | 0.100 | 13.98 (0.05) | 13.35 (0.05) | 3757 (300) | 10, 11, 12 |
| 2001du | NGC 1365 | 1636 | 17.95 (0.41) | 0.170 | 15.00 (0.10) | 14.35 (0.10) | 3980 (220) | 1, 13, 14 |
Notes. The SNe are ordered in terms of increasing distance. 1) Distance from Freedman et al. (2001); 2) magnitudes and velocity from Vinkó et al. (2006); 3) reddening from Meikle et al. (2011); 4) distance from Pietrzyński et al. (2010); 5) magnitudes from Pignata (2013); 6) velocity measured from spectrum downloaded from the ESO archive; 7) distance from Fiorentino et al. (2013); 8) magnitudes, reddening and velocity from Dall’Ora et al. (2014); 9) velocity measured from spectrum downloaded from Weizmann Interactive Supernova Data Repository (WISeREP; Yaron & Gal-Yam 2012; http://www.weizmann.ac.il/astrophysics/wiserep/); 10) distance from Leonard et al. (2003); 11) magnitudes and velocity from Hamuy (2003b); 12) reddening from Elmhamdi et al. (2003); 13) velocity measured from spectrum in Smartt et al. (2003) who also estimate the reddening; 14) magnitudes from Van Dyk et al. (2003).
Velocities extrapolated to 50 days using Eq. (2) of Nugent et al. (2006).
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