Table 1
SN sample used in this analysis.
| SN | tB(max) | Δm15(B) | s BV | sBV reference | t2(Y) 1 | t2(J) | μ | Distance method ** | Distance reference | Data reference | |
| (MJD; d) | (mag) | (d) | (mag) | ||||||||
|
|
|||||||||||
| SN1999by * 2 | 51 308.3 | 1.93 | 0.46 | This paper | N/A | N/A | 30.82 (±0.15) | TF | T13 | H02, G04 | |
| SN2003gs | 52 848.3 | 1.83 | 0.49 | This paper | ··· | 15.3 (±0.7) | 31.65 (±0.28) | SBF | T01 | K09 | |
| SN2005bl * | 53 481.6 | 1.80 | 0.39 | B14 | N/A | N/A | 35.14 (±0.09) | LD | WV08, F15 | ||
| SN2005ke * | 53 698.6 | 1.78 | 0.41 | B14 | N/A | ··· | 31.84 (±0.08) | SBF | T01 | WV08, C10, F15 | |
| SN2006gt* | 54 003.1 | 1.66 | 0.56 | B14 | ··· | 20.2 (±1.2) | 36.43 (±0.05) | LD | C10 | ||
| SN2006mr * | 54 050.2 | 1.84 | 0.26 | B14 | N/A | N/A | 31.15 (±0.23) | SBF | A01 | C10 | |
| SN2007N * | 54 124.3 | 1.79 | 0.29 | B14 | N/A | N/A | 33.91 (±0.16) | LD | S11 | ||
| SN2007ax * | 54 187.5 | 1.86 | 0.36 | B14 | N/A | N/A | 32.20 (±0.14) | TF | T09 | S11 | |
| SN2007ba* | 54 196.2 | 1.88 | 0.54 | B14 | 20.0 (±0.4) | ··· | 36.18 (±0.05) | LD | S11 | ||
| SN2007on | 54 421.1 | 1.90 | 0.57 | B14 | 18.7 (±0.4) | 18.2 (±0.1) | 31.45 (±0.08) | SBF | J03 | S11 | |
| SN2008R* | 54 494.3 | 1.85 | 0.59 | B14 | 15.5 (±0.7) | 14.1 (±0.7) | 33.73 (±0.16) | LD | S11 | ||
| SN2008hs | 54 812.1 | 1.83 | 0.60 | This paper | ··· | 14.0 (±1.0) | 34.28 (±0.13) | LD | F15 | ||
| SN2009F * | 54 841.8 | 1.97 | 0.33 | B14 | N/A | N/A | 33.73 (±0.16) | LD | S11 | ||
| SN2010Y | 55 247.5 | 1.73 | 0.61 | This paper | ··· | ··· | 33.44 (±0.20) | LD | F15 | ||
| iPTF13ebh | 56 622.9 | 1.79 | 0.63 | H15 | 19.4 (±0.2) | 17.2 (±1.5) | 33.63 (±0.16) | LD | H15 | ||
Notes. TF, Tully-Fisher relation; and SBF, surface brightness fluctuation. We wish to note that 0.16 mag (Jensen et al. 2003) is subtracted from SBF distances from Tonry et al. (2001) to put them on the same scale as Freedman et al. (2001). We wish to note that objects that do not have a luminosity distance presented here are not in the Hubble flow, meaning they have z< 0.01.
SN Ia with only one maximum are marked as “N/A”. Ellipses indicate insufficient data to determine a second maximum.
Methods for distances to the SN hosts are as follows: LD, luminosity distance (using parameters detailed in the text);
Reference. A01: Ajhar et al. (2001); T01: Tonry et al. (2001); H02: Höflich et al. (2002); J03: Jensen et al. (2003); G04: Garnavich et al. (2004); K09: Krisciunas et al. (2009); WV08: Wood-Vasey et al. (2008); C10: Contreras et al. (2010); S11: Stritzinger et al. (2011); T09: Tully et al. (2009); T13: Tully et al. (2013); F15: Friedman et al. (2015); H15: Hsiao et al. (2015).
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