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

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Table 5

Significant K-S statistics and correlations for NaIDVEL divided according to galaxy properties.

Property	Nr	$< D_{M C}^{V E L} >$ $<D^{\mathrm{VEL}}_{\mathrm{MC}}>$	$< p_{M C}^{V E L} >$ $<p_{\mathrm{MC}}^{\mathrm{VEL}}>$	P	$r_{s}^{V E L}$ $r_s^{\mathrm{VEL}}$
Δα	462	0.16	0.011	71%	−0.08

Notes. Similar to Table 4 for the NaI D VEL (for SNe with EW> |0.3|Å) only for galaxy properties with low K-S p-values (P > 35%) and significantly low p-values highlighted in bold (P > 50%). Values for the MW lines are not shown, but are consistent with being drawn from the same parent population.

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