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Table 5

Comparison between our 1D 1σ confidence regions for the CMF and those of Barr et al. (2018).

Planet CMF

Barr et al. (2018) This study (2020)
b 0.00–0.43 0.12–0.41
c 0.00–0.98 0.16–0.32
d 0.00–0.39 0.24–0.58
e 0.00–0.40 0.32–0.57
f 0.00 0.24–0.58
g 0.00 0.26–0.54
h 0.00 0.15–0.53

Notes. We show only estimates for scenario 1, because Barr et al. (2018) did not consider any constraints on the Fe/Si ratio based on stellar composition.

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