Table 3
Log evidence values for the different models.
Model | ln 𝒵 | ||||
---|---|---|---|---|---|
GJ 832 | GJ 674 | Ross 128 | Ross 128 | Ross 128 | |
HARPS All | HARPS All | HARPS All | HARPS RedDots | HARPS All + CARMENES | |
0P | −702.819 | −872.623 | −732.539 | −329.860 | −879.788 |
ipecc | −417.245 | −721.134 | −726.180 | −329.607 | −861.687 |
1 Pcirc | −414.969 | −711.435 | −716.440 | −329.813 | −859.088 |
2Pecc | −431.104 | −675.651 | −729.838 | −334.821 | −885.959 |
2Pcirc | −408.309 | −714.733 | −725.025 | −308.788 | −868.615 |
0P + GP−SHO | −427.620 | −856.580 | −638.419 | −281.841 | −781.387 |
0P + GP−dSHO | −433.437 | −720.755 | −659.400 | −290.842 | −805.854 |
0P + GP−QP | −399.979 | −687.511 | −648.438 | −284.849 | −791.900 |
1Pecc + GP−SHO | −369.321 | −593.106 | −624.030 | −284.425 | −761.586 |
1Pcirc + GP−SHO | −365.269 | −670.372 | −623.183 | −283.352 | −760.829 |
1Pecc + GP−dSHO | −373.048 | −583.193 | −631.783 | −289.003 | −774.871 |
1Pcirc+ GP−dSHO | −371.079 | −648.977 | −631.608 | −289.949 | −776.500 |
1Pecc + GP−QP | −371.120 | −590.442 | −636.535 | −289.520 | −774.581 |
1Pcirc + GP−QP | −368.356 | −711.195 | −634.859 | −287.351 | −773.571 |
2Pecc + GP−SHO | −372.301 | −797.946 | −650.356 | −286.935 | −786.794 |
2Pcirc + GP−SHO | −370.827 | −667.461 | −624.541 | −288.612 | −763.897 |
2Pecc + GP−dSHO | −382.833 | −824.353 | −685.895 | −290.482 | −814.590 |
2Pcirc + GP−dSHO | −375.092 | −681.185 | −664.176 | −291.211 | −809.106 |
2Pecc + GP−QP | −385.800 | −701.913 | −665.416 | −294.656 | −830.340 |
2Pcirc + GP−QP | −372.643 | −682.551 | −678.288 | −292.517 | −781.612 |
Notes. We used models with zero, one, and two planets; with and without GP; using the SHO, dSHO or QP kernels. The highest evidence per column is marked in bold. Multiple entries are marked where the values are considered indistinguishable at ∆ ln 𝒵 < 5. The entries marked in bold italics refer to the models we prefer from Sects. 5.1.1–5.1.3 even though for GJ 674 this is a model with ∆ ln 𝒵 > 5. Our reasoning is given in Sect. 5.1.2.
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