The radial distribution of core-collapse supernovae in spiral host galaxies

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Table 5:

Kolmogorov-Smirnov tests of the consistency of the radial distributions of CCSNe among different pairs of subsamples.
Subsample 1	Subsample 2	$\tilde{P}_{\rm KS}$	$\hat{P}_{\rm KS}$
(1)	(2)	(3)	(4)
Sc-Sd	Sa-Sbc	0.935	0.300
Sa-Sbc (SNe Ib/c)	Sc-Sd (SNe Ib/c)	0.197	0.110
Sc-Sd (SNe II)	Sa-Sbc (SNe II)	0.926	0.268
Sa-Sd (without bars)	Sa-Sd (with bars)	0.398	0.214
Sa-Sbc (with bars)	Sa-Sbc (without bars)	0.711	0.313*
Sc-Sd (without bars)	Sc-Sd (with bars)	0.294	0.282
$-23 < M_{\rm disk} \leq -20.5$	$-20.5 < M_{\rm disk} < -18$	0.114	0.006
$19.65 < \mu_0^{\rm disk} \leq 20.60$	$20.60 < \mu_0^{\rm disk} < 21.85$	0.469	0.723*
$0^\circ \leq i \leq 30^\circ$	$30^\circ < i \leq 50^\circ$	0.273	0.050
$V_{\rm r}\leq5000$	$V_{\rm r}>5000$	0.992*	0.568
$V_{\rm r}\leq5000$ (SNe Ib/c)	$V_{\rm r}>5000$ (SNe Ib/c)	0.444*	0.475*
$V_{\rm r}\leq5000$ (SNe II)	$V_{\rm r}>5000$ (SNe II)	0.924*	0.674
SNe Ic	SNe Ib	0.946	0.751*
SNe Ib	SNe II	0.055	0.156
SNe Ic	SNe II	0.006	0.035
SNe Ib/c	SNe II	0.002	0.015

Notes: Column 1: more radially concentrated subsample; Col. 2: less radially concentrated subsample (the contrary cases are marked by asterisks). CCSN distributions inconsistent within two subsamples are highlighted in bold.

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