A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE - I. Sample selection, analysis of local environments, and correlations with light curve properties

Open Access

Fig. 8.

Cumulative distributions of the line of sight extinction E(B − V), estimated from the Balmer decrement. The top row shows the distributions for the different types of CCSNe, while the bottom row shows the distributions for the CCSNe grouped into SNe II, SESNe, and IIn/Ibn. The right column shows the Kolmogorov–Smirnov (KS) statistic matrix.

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