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Fig. 11

image

E(VXλ)host as a function of wavelength for seven objects whose E(VB)host< −0.20 mag and with 8 different E(VXλ)host combinations extending from E(Vu)host to E(VH)host (except for SN 2009dt where uV is missing). Diamonds correspond to E(VXλ)host values obtained by comparison with the intrinsic color-curve templates for each object’s spectroscopic sub-type. Solid lines represent the best reddening law fit to each series of data and the corresponding 1σ uncertainty of the fit is indicated with dashed lines. The SN names are color coded with respect to their spectroscopic sub-type, i.e. SNe IIb in green, SNe Ib in blue, SNe Ic in red, and SNe Ic-BL in magenta.

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