Mid-IR water and silicate relation in protoplanetary disks

S. Antonellini; J. Bremer; I. Kamp; P. Riviere-Marichalar; F. Lahuis; W.-F. Thi; P. Woitke; R. Meijerink; G. Aresu; M. Spaans

doi:10.1051/0004-6361/201527820

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Volume 597 (January 2017)

A&A, 597 (2017) A72

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Table 2

Kolmogorov-Smirnov, Anderson-Darling, and Mantel-Haenszel test results.

Data	KS	AD	MH
	p-value^*	p-value^*	p-value^*

Peak 10 μm	6.921 × 10^-7	2.457 × 10^-6	n.a.
Water 15.17 μm	0.246	0.163	0.166
Water 17.22 μm	0.285	0.189	0.173
Water 29.85 μm	0.936	0.696	0.774

Notes.

^(*)

p-value represents the coefficient that determines whether we can discard the null hypothesis (samples pertain to the same distribution if p> 0.05 for KS and AD, and p> 0.1 for MH.)

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