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Table 4:

Results of the K-S and R-S tests on different subsets of systems.
Sub-sample D Pr(D) Z Pr(Z)
Eccentricity distribution
1 vs. 2 0.435 0.002 3.142 0.001
1 vs. 4 0.50 0.08 2.18 0.01
1 vs. 3+4 0.449 0.001 3.4535 0.0003
2 vs. 4 0.32 0.64 0.73 0.23
2 vs. 3+4 0.21 0.65 0.24 0.41
Metallicity distribution
1 vs. 2 0.22 0.27 -0.67 0.25
1 vs. 4 0.46 0.06 -1.57 0.06
1 vs. 3+4 0.389 0.002 -2.745 0.007
2 vs. 4 0.31 0.51 -1.11 0.13
2 vs. 3+4 0.28 0.23 -1.36 0.09

Notes. All planets from the Butler et al. 2006 catalog with $M_{\rm c}\sin i< 4$$M_{\rm J}$(1), companions with $4 < M_{\rm c}\sin i< 10$ $M_{\rm J}$(2), companions with $10 < M_{\rm c} \sin i< 80 $ $M_{\rm J}$but excluding those with confirmed mass higher than 80 $M_{\rm J}$ (3), and companions with true masses in the range $10 < M_{\rm c}< 80$$M_{\rm J}$(4).


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