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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
(1),
companions with
(2),
companions with
but
excluding those with confirmed mass higher than 80
(3),
and companions with true masses in the range
(4).
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