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

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Table 2

Galaxy properties studied.

Property	Description	Reference
Type	Galaxy classification	NED^*/Asiago
Δα(°)	SN angular offset	Eq. (1)
$\bar{Δ α}$ $\overline{\Delta\alpha}$	SN normalised offset	Eq. (2)
Δα_DLR	SN directional offset	Eq. (4)
i(°)	Galaxy inclination	Eq. (5)
$M_{}^{G} / M_{⊙}$ $M_^G/M_{\odot}$	Global stellar mass	Sect. 2.2.2
$Z_{}^{G} / Z_{⊙}$ $Z_^G/Z_{\odot}$	Global stellar metallicity	Sect. 2.2.2
$t_{a g e}^{G} (G y r)$ $$t_{\mathrm{age}}^G$(Gyr)$	Global age	Sect. 2.2.2
τ^G(Gyr)	Global e-folding time	Sect. 2.2.2
$A_{V}^{G}$	Global attenuation	Sect. 2.2.2
n^G	Global dust index	Sect. 2.2.2
$S F R_{0}^{G} (M_{⊙} / y r)$ $SFR$_0^G (M_{\odot}$/yr)$	Global SFR	Eq. (6)
$s S F R_{0}^{G} (y r^{- 1})$ $sSFR$_0^G$ (yr$^{-1}$)$	Global specific SFR	Eq. (8)
$M_{}^{L} / M_{⊙}$ $M_^L/M_{\odot}$	Local stellar mass	Sect. 2.2.2
$Z_{}^{L} / Z_{⊙}$ $Z_^L/Z_{\odot}$	Local stellar metallicity	Sect. 2.2.2
$t_{a g e}^{L} (G y r)$ $$t_{\mathrm{age}}^L$(Gyr)$	Local age	Sect. 2.2.2
$τ^{L} (G y r)$ $$\tau^L$(Gyr)$	Local e-folding time	Sect. 2.2.2
$A_{V}^{L}$	Local attenuation	Sect. 2.2.2
n^L	Local dust index	Sect. 2.2.2
$S F R_{0}^{L} (M_{⊙} / y r)$ $SFR$_0^L (M_{\odot}$/yr)$	Local SFR	Eq. (6)
$s S F R_{0}^{L} (y r^{- 1})$ $sSFR$_0^L$ (yr$^{-1}$)$	Local specific SFR	Eq. (8)

Notes. ^*We use the NED homogenised classification scheme.

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