Table B.1
Overview of the distributions of retrieved planetary radii when comparing different baseline models.
Magnitude | Impact Parameter | FB | P2 | SP | MGP | SGP |
---|---|---|---|---|---|---|
8.5 | 0.0 | 1.08 ± 0.07 | 1.00 ± 0.07 | 1.00 ± 0.08 | 1.04 ± 0.06 | 1.08 ± 0.07 |
0.25 | 1.08 ± 0.07 | 1.02 ± 0.06 | 1.02 ± 0.06 | 1.04 ± 0.06 | 1.07 ± 0.07 | |
0.5 | 1.06 ± 0.07 | 1.01 ± 0.07 | 1.00 ± 0.07 | 1.04 ± 0.06 | 1.05 ± 0.07 | |
0.75 | 1.08 ± 0.08 | 0.99 ± 0.08 | 0.99 ± 0.08 | 1.04 ± 0.08 | 1.08 ± 0.08 | |
0.9 | 1.07 ± 0.14 | 1.01 ± 0.07 | 1.02 ± 0.07 | 1.02 ± 0.09 | 1.06 ± 0.13 | |
all | 1.07 ± 0.07 | 1.01 ± 0.07 | 1.01 ± 0.07 | 1.04 ± 0.06 | 1.07 ± 0.07 | |
9.5 | 0.0 | 1.17 ± 0.13 | 0.99 ± 0.12 | 0.99 ± 0.13 | 1.03 ± 0.08 | 1.17 ± 0.13 |
0.25 | 1.14 ± 0.14 | 1.03 ± 0.10 | 1.04 ± 0.10 | 1.03 ± 0.07 | 1.15 ± 0.13 | |
0.5 | 1.11 ± 0.12 | 0.99 ± 0.09 | 1.00 ± 0.10 | 1.00 ± 0.08 | 1.12 ± 0.12 | |
0.75 | 1.11 ± 0.12 | 1.03 ± 0.08 | 1.03 ± 0.07 | 1.02 ± 0.08 | 1.11 ± 0.11 | |
0.9 | 1.03 ± 0.19 | 1.03 ± 0.12 | 1.02 ± 0.11 | 1.01 ± 0.10 | 1.02 ± 0.15 | |
all | 1.14 ± 0.13 | 1.02 ± 0.11 | 1.02 ± 0.10 | 1.02 ± 0.08 | 1.13 ± 0.12 | |
10.5 | 0.0 | 1.26 ± 0.22 | 1.05 ± 0.18 | 1.04 ± 0.20 | 1.04 ± 0.09 | 1.26 ± 0.20 |
0.25 | 1.31 ± 0.24 | 1.07 ± 0.18 | 1.08 ± 0.20 | 1.05 ± 0.11 | 1.31 ± 0.24 | |
0.5 | 1.24 ± 0.21 | 1.06 ± 0.20 | 1.07 ± 0.19 | 1.01 ± 0.10 | 1.24 ± 0.18 | |
0.75 | 1.27 ± 0.20 | 1.04 ± 0.17 | 1.05 ± 0.14 | 1.01 ± 0.13 | 1.26 ± 0.24 | |
0.9 | 1.18 ± 0.25 | 1.10 ± 0.24 | 1.09 ± 0.21 | 0.96 ± 0.21 | 1.18 ± 0.24 | |
all | 1.25 ± 0.20 | 1.06 ± 0.17 | 1.06 ± 0.18 | 1.03 ± 0.10 | 1.26 ± 0.20 | |
11.5 | 0.0 | 1.46 ± 0.36 | 1.05 ± 0.25 | 1.04 ± 0.24 | 1.12 ± 0.17 | 1.44 ± 0.40 |
0.25 | 1.55 ± 0.47 | 0.97 ± 0.32 | 0.99 ± 0.25 | 1.01 ± 0.14 | 1.54 ± 0.45 | |
0.5 | 1.55 ± 0.47 | 1.15 ± 0.34 | 1.11 ± 0.31 | 1.05 ± 0.14 | 1.50 ± 0.39 | |
0.75 | 1.42 ± 0.28 | 1.10 ± 0.25 | 1.10 ± 0.23 | 1.05 ± 0.19 | 1.43 ± 0.27 | |
0.9 | 1.33 ± 0.37 | 1.02 ± 0.21 | 0.98 ± 0.26 | 0.93 ± 0.14 | 1.36 ± 0.35 | |
all | 1.46 ± 0.34 | 1.06 ± 0.26 | 1.05 ± 0.26 | 1.05 ± 0.16 | 1.47 ± 0.34 | |
12.5 | 0.0 | Upp. boundary | 0.97 ± 0.41 | 1.01 ± 0.46 | 1.28 ± 0.30 | 1.66 ± 0.41 |
0.25 | Upp. boundary | 0.96 ± 0.60 | 0.97 ± 0.60 | 1.25 ± 0.20 | 1.61 ± 0.35 | |
0.5 | Upp. boundary | 0.96 ± 0.47 | 0.98 ± 0.45 | 1.18 ± 0.38 | 1.82 ± 0.45 | |
0.75 | Upp. boundary | 1.05 ± 0.69 | 1.05 ± 0.71 | 1.12 ± 0.29 | 1.60 ± 0.33 | |
0.9 | Upp. boundary | 0.90 ± 0.56 | 0.91 ± 0.52 | 1.05 ± 0.37 | 1.72 ± 0.42 | |
all | Upp. boundary | 0.98 ± 0.53 | 0.99 ± 0.54 | 1.21 ± 0.31 | 1.67 ± 0.35 |
Notes. The medians and standard deviations of 88 retrieved planetary radii Rpl for different combinations of stellar magnitudes, impact parameters, and baseline models are shown. Upp. Boundary indicates that the majority of fitting runs ended up at or near the upper boundary of the uniform prior constraining the parameter.
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