The Herschel Gould Belt Survey in Chamaeleon II - Properties of cold dust in disks around young stellar objects

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Table 4

Results of the 2D Kolmogorov-Smirnov test comparing the distribution of YSOs and galaxies in PACS/SPIRE CC diagrams (Fig. 4).

CC diagram	Probability^†	Probability^†	Probability^†
	Cha II vs.	Cha I vs.	Serpens vs.
	galaxies	galaxies	galaxies

F₂₅₀/F₃₅₀ vs. F₇₀/F₁₆₀	6.e-06	3.e-09	7.e-06
F₂₅₀/F₃₅₀ vs. F₁₆₀/F₂₅₀	2.e-07	8.e-07	6.e-07
F₂₅₀/F₃₅₀ vs. F₃₅₀/F₅₀₀	4.e-07	7.e-09	2.e-08

Notes.

^(†)

The computed probability is 1 for two populations drawn from same parent distribution, and 0 for two populations with ideally different distributions.

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