Table E.4
K-S statistics and correlations for Na I D EW and VEL in SNe Ia-pass divided according to galaxy properties.
| EW | VEL | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Property | Nr | ![]() |
![]() |
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Nr | ![]() |
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| General properties | ||||||||||
| T-type† | 139 | 0.40 | 3.31×10−4 | 91% | 0.35 | 71 | 0.27 | 2.66×10−1 | 10% | −0.10 |
| Δα | 133 | 0.36 | 1.79×10−3 | 91% | −0.30 | 69 | 0.34 | 9.07×10−2 | 25% | −0.18 |
| Δα(°) | 131 | 0.38 | 2.33×10−3 | 87% | −0.28 | 70 | 0.27 | 3.15×10−1 | 8% | −0.13 |
| ΔαDLR | 133 | 0.35 | 3.00×10−3 | 80% | −0.27 | 69 | 0.40 | 2.21×10−1 | 49% | −0.19 |
| i(°) | 133 | 0.16 | 4.82×10−1 | 3% | 0.03 | 69 | 0.32 | 1.42×10−1 | 18% | 0.14 |
| Global properties | ||||||||||
| nG | 130 | 0.25 | 7.01×10−2 | 30% | 0.18 | 71 | 0.24 | 4.24×10−1 | 5% | −0.15 |
| M*G/M⊙ | 130 | 0.17 | 4.16×10−1 | 7% | −0.12 | 71 | 0.26 | 3.31×10−1 | 5% | −0.04 |
| Z*G/Z⊙ | 130 | 0.19 | 3.32×10−1 | 6% | −0.04 | 71 | 0.35 | 4.18×10−1 | 4% | 0.09 |
| SFR0G (M⊙/yr) | 130 | 0.18 | 3.80×10−1 | 5% | −0.04 | 71 | 0.29 | 2.80×10−1 | 8% | −0.08 |
| AVG | 130 | 0.19 | 3.88×10−1 | 5% | 0.04 | 71 | 0.24 | 5.35×10−1 | 3% | −0.10 |
| tageG(Gyr) | 130 | 0.16 | 5.30×10−1 | 2% | −0.05 | 71 | 0.24 | 4.74×10−1 | 3% | 0.06 |
| τG(Gyr) | 130 | 0.15 | 5.55×10−1 | 2% | 0.01 | 71 | 0.26 | 3.20×10−1 | 6% | −0.09 |
| sSFR0G (yr−1) | 130 | 0.16 | 5.19×10−1 | 2% | 0.04 | 71 | 0.27 | 3.13×10−1 | 6% | −0.01 |
| Local properties | ||||||||||
| SFR0L (M⊙/yr) | 51 | 0.47 | 5.02×10−2 | 36% | 0.25 | 23 | 0.50 | 5.45×10−1 | 2% | 0.18 |
| M*L/M⊙ | 51 | 0.36 | 1.64×10−1 | 16% | 0.26 | 23 | 0.50 | 3.03×10−1 | 8% | 0.41 |
| τL(Gyr) | 51 | 0.32 | 2.56×10−1 | 10% | −0.06 | 23 | 0.47 | 4.08×10−1 | 5% | −0.10 |
| sSFR0L (yr−1) | 51 | 0.34 | 2.97×10−1 | 9% | 0.08 | 23 | 0.50 | 5.38×10−1 | 2% | −0.07 |
| nL | 51 | 0.32 | 2.91×10−1 | 9% | 0.09 | 23 | 0.55 | 3.64×10−1 | 5% | 0.29 |
| tageL (Gyr) | 51 | 0.30 | 3.93×10−1 | 5% | −0.09 | 23 | 0.55 | 3.29×10−1 | 6% | 0.19 |
| Z*L/Z⊙ | 51 | 0.27 | 4.89×10−1 | 2% | −0.01 | 23 | 0.47 | 4.60×10−1 | 3% | 0.24 |
| AVL | 51 | 0.27 | 4.35×10−1 | 4% | 0.06 | 23 | 0.44 | 4.94×10−1 | 3% | 0.10 |
Notes. The null hypothesis probed by the K-S test is that the Na I D EW of two samples divided according to a value between the 40% and 60% percentile of the galaxy property indicated in the leftmost column of Table 2 in Paper II comes from the same parent population. The K-S statistic, D, the p-value, the probability P of the p value being lower than 0.05, and the correlation rs are shown. Significant rejections of the hypothesis (
) are highlighted in bold.
Galaxy properties: T-type: Galaxy classification; ∆α: SN normalised offset; ∆αDLR: SN directional offset; ∆α(°): SN angular offset; i(°): Galaxy inclination; M*: Stellar mass; SFR: Star formation rate; sSFR: Specific SFR; Z*: Stellar metallicity; tage: Age; AV: Attenuation; n: dust index; τ: e-folding time.
*This probability is obtained from the median of 1000 bootstrap ’z-matched’ simulations on the two samples recalculating the K-S statistic at each iteration and additionally dividing the sample in two at 10 different positions around the median (40-60% percentile).
†The T-type samples are divided between spirals and ellipticals (at a fixed T-type = 0) instead of the range around the median (<T-type>~ 2).
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