RV from multiwaveband galaxy polarimetry in the vicinity of supernovae

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Table C.1

R_V estimates of SNe inferred using INLA.

SN	Host Galaxy	$λ_{\max}^{I N L A}$ $\lambda _{\max }^{INLA}$ (µm)	$R_{V} (λ_{\max}^{I N L A})$ ${{\rm{R}}_V}\left( {\lambda _{\max }^{INLA}} \right)$	$R_{V}^{I N L A}$ $R_V^{INLA}$	∆R_V (σ)	Projected Area (kpc²)
2011iv	NGC-1404	0.55 ± 0.15	3.09 ± 0.85	3.23 ± 0.79	0.12	0.12 × 0.12
2010ev	NGC-3244	0.57 ± 0.59	3.2 ± 3.3	3.42 ± 0.89	0.08	0.17 × 0.17
2012cg	NGC-4424	0.58 ± 0.34	3.3 ± 1.9	3.17 ± 0.73	0.04	0.09 × 0.09
2007le	NGC-7721	0.48 ± 0.27	2.7 ± 1.5	3.18 ± 0.83	0.28	0.13 × 0.13
2001da	NGC-7780	0.60 ± 0.69	3.3 ± 3.9	3.9 ± 1.0	0.15	0.45 × 0.45
2006cm	UGC-11723	0.58 ± 0.54	3.3 ± 3.0	3.43 ± 0.87	0.05	0.43 × 0.43
2007fb	UGC-12859	0.6 ± 1.3	3.5 ± 7.3	3.7 ± 1.3	0.02	1.36 × 1.36

Notes. In column three we provide $λ_{m a x}^{I N L A}$ $\lambda _{max}^{INLA}$ , obtained with spatial inference of the previously obtained bin maps of λ_max, for the vicinity of the SNe hosted by the galaxies in our sample; while in column four we present the $R_{V} (λ_{m a x}^{I N L A})$ ${{\rm{R}}_V}\left( {\lambda _{max}^{INLA}} \right)$ , calculated using the $λ_{m a x}^{I N L A}$ $\lambda _{max}^{INLA}$ values and Eq. (10). In column five $R_{V}^{I N L A}$ $R_V^{INLA}$ is obtained with spatial inference of the previously obtained bin maps of R_V. In column six we present the difference between $R_{V} (λ_{m a x}^{I N L A})$ ${{\rm{R}}_V}\left( {\lambda _{max}^{INLA}} \right)$ and $R_{V}^{I N L A}$ $R_V^{INLA}$ . ∆R_V is given in σ. The projected area, in kpc², corresponding to the bin selection is provided in column seven.

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