Narrow absorption lines from intervening material in supernovae - II. Galaxy properties

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Table 6

Significant K-S statistics and correlations for the EW and VEL of narrow lines (other than NaI D ) divided according to galaxy properties.

Property	Nr	<D_MC>	<p_MC>	P	r_s
Host CaII H EW
$\bar{Δ α}$ $\boldsymbol{$\overline{\Delta\alpha}$}$	226	0.29	6.6×10⁻⁴	92%	−0.27
$M_{}^{L}$ ${\bf M$_^L$}$	137	0.29	0.014	62%	0.19
$S F R_{0}^{L}$ $\bf{SFR$_0^L$}$	137	0.30	9.7×10⁻³	70%	0.28
$s S F R_{0}^{L}$ $\bf{sSFR$_0^L$}$	137	0.28	0.022	54%	0.27
$t_{a g e}^{L}$ $\boldsymbol{$t_{\mathrm{age}}^L$}$	137	0.29	0.013	60%	−0.21
Host CaII K EW
$\bar{Δ α}$ $\boldsymbol{$\overline{\Delta\alpha}$}$	170	0.25	0.024	58%	−0.26
$S F R_{0}^{L}$ $\bf{SFR$_0^L$}$	106	0.36	7.0×10⁻³	77%	0.16
$s S F R_{0}^{L}$	106	0.32	0.031	49%	0.21
$t_{a g e}^{L}$ $\boldsymbol{$t_{\mathrm{age}}^L$}$	106	0.34	0.010	69%	−0.24
Host CaII K VEL
i(°)	113	0.30	0.038	43%	0.20
Host KI 1 EW
$\bar{Δ α}$ $\boldsymbol{$\overline{\Delta\alpha}$}$	437	0.21	3.9×10⁻⁴	96%	−0.22
$M_{}^{L}$ ${\bf M$_^L$}$	281	0.20	0.019	58%	0.16
$S F R_{0}^{L}$ $\bf{SFR$_0^L$}$	281	0.24	2.0×10⁻³	85%	0.18
Host DIB 5780 EW
$\bar{Δ α}$ $\boldsymbol{$\overline{\Delta\alpha}$}$	488	0.20	6.2×10⁻⁴	92%	−0.12
$M_{*}^{L}$	303	0.18	0.032	47%	0.16
$A_{V}^{L}$	303	0.17	0.046	40%	0.17
$M_{}^{G}$ $\boldsymbol{$M_^G$}$	466	0.16	0.015	62%	0.16
$t_{a g e}^{G}$ $\boldsymbol{$t_{\mathrm{age}}^G$}$	466	0.16	0.012	58%	0.08
Host DIB 5780 VEL
$M_{*}^{L}$	113	0.29	0.039	40%	0.25
$A_{V}^{G}$	208	0.22	0.034	47%	−0.09
Host DIB 6283 EW
T-type	560	0.21	0.040	49%	0.11
$t_{a g e}^{L}$ $t_{\mathrm{age}}^L$	342	0.17	0.041	41%	−0.12
*n^L*	342	0.18	0.020	58%	0.14

Notes. Similar to Table 4 for Ca II H&K, K I 1 & 2 and the DIB 5780, 4428 and 6283 lines only for galaxy properties with low K-S p-values (P > 40%) and significantly low p-values (P > 50%) highlighted in bold. Values for the MW lines are not shown, but are consistent with being drawn from the same parent population.

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