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Table H.1
Estimated planet masses for each observed gap using the Kanagawa et al. (2016) model.
| System | Gap Width (au) | (au) | hp/rp | Mp (MJ) (αvisc = 10−2) | Mp (MJ) (αvisc = 10−3) | Mp (MJ) (αvisc = 10−4) |
|---|---|---|---|---|---|---|
| J16120668-3010270 | 61.4 ± 0.6 | 61.1 ± 0.3 | 0.019 | 1.11 ± 1.13 | 0.35 ± 0.36 | 0.11 ± 0.11 |
| J18521730-3700119 | 34.3 ± 0.5 | 48.5 ± 0.2 | 0.016 | 0.61 ± 0.73 | 0.19 ± 0.23 | 0.06 ± 0.07 |
| HD 97048 | 80.2 ± 1.2 | 156.2 ± 0.6 | 0.026 | 1.73 ± 1.26 | 0.55 ± 0.40 | 0.17 ± 0.13 |
| 75.0 ± 6.7 | 233.8 ± 3.3 | 0.030 | 0.83 ± 0.55 | 0.26 ± 0.17 | 0.08 ± 0.05 | |
| 97.1 ± 10.0 | 319.9 ± 5.0 | 0.033 | 0.87 ± 0.53 | 0.28 ± 0.17 | 0.09 ± 0.05 | |
| HD 169142 | 33.1 ± 0.4 | 51.8 ± 0.2 | 0.016 | 0.89 ± 1.02 | 0.28 ± 0.32 | 0.09 ± 0.10 |
| HD 34282 | 58.5 ± 2.2 | 201.4 ± 1.1 | 0.044 | 0.76 ± 0.34 | 0.24 ± 0.11 | 0.08 ± 0.03 |
| 86.3 ± 5.2 | 273.8 ± 2.6 | 0.054 | 1.25 ± 0.47 | 0.39 ± 0.15 | 0.12 ± 0.05 | |
| IM Lup | 65.8 ± 0.5 | 138.6 ± 0.2 | 0.047 | 1.42 ± 0.59 | 0.45 ± 0.19 | 0.14 ± 0.06 |
| 61.8 ± 2.7 | 202.4 ± 1.4 | 0.053 | 0.71 ± 0.27 | 0.22 ± 0.08 | 0.07 ± 0.03 | |
| 121.7 ± 4.8 | 294.2 ± 2.4 | 0.060 | 1.55 ± 0.53 | 0.49 ± 0.17 | 0.15 ± 0.05 | |
| RXJ1615-3255 | 75.9 ± 1.2 | 107.8 ± 0.6 | 0.023 | 1.17 ± 0.97 | 0.37 ± 0.31 | 0.12 ± 0.10 |
| 58.0 ± 1.3 | 174.8 ± 0.6 | 0.034 | 0.47 ± 0.26 | 0.15 ± 0.08 | 0.05 ± 0.03 | |
| 73.7 ± 1.7 | 240.6 ± 0.9 | 0.043 | 0.58 ± 0.26 | 0.18 ± 0.08 | 0.06 ± 0.03 | |
| TW Hya | 14.3 ± 0.3 | 29.1 ± 0.2 | 0.011 | 0.14 ± 0.24 | 0.05 ± 0.08 | 0.01 ± 0.02 |
| 12.0 ± 0.3 | 42.2 ± 0.2 | 0.015 | 0.07 ± 0.09 | 0.02 ± 0.03 | 0.01 ± 0.01 | |
| 21.0 ± 0.3 | 58.7 ± 0.2 | 0.018 | 0.16 ± 0.16 | 0.05 ± 0.05 | 0.02 ± 0.02 | |
| 41.1 ± 0.6 | 89.8 ± 0.3 | 0.025 | 0.40 ± 0.31 | 0.13 ± 0.10 | 0.04 ± 0.03 | |
| 48.2 ± 1.5 | 134.4 ± 0.8 | 0.033 | 0.38 ± 0.22 | 0.12 ± 0.07 | 0.04 ± 0.02 | |
| V4046 Sgr | 14.3 ± 0.1 | 24.7 ± 0.0 | 0.004 | 0.11 ± 0.46 | 0.03 ± 0.15 | 0.01 ± 0.05 |
| 20.8 ± 0.6 | 42.3 ± 0.3 | 0.014 | 0.44 ± 0.60 | 0.14 ± 0.19 | 0.04 ± 0.06 | |
| WISPIT 2 (H-band) | 58.3 ± 0.6 | 67.6 ± 0.3 | 0.018 | 1.20 ± 1.26 | 0.38 ± 0.40 | 0.12 ± 0.13 |
| 66.8 ± 3.0 | 130.1 ± 1.5 | 0.030 | 0.93 ± 0.59 | 0.29 ± 0.19 | 0.09 ± 0.06 | |
| 152.8 ± 5.4 | 240.0 ± 2.7 | 0.049 | 2.94 ± 1.19 | 0.93 ± 0.38 | 0.29 ± 0.12 | |
| WISPIT 2 (K-band) | 65.5 ± 1.4 | 70.0 ± 0.7 | 0.011 | 0.66 ± 1.15 | 0.21 ± 0.36 | 0.07 ± 0.12 |
| 53.6 ± 2.2 | 129.5 ± 1.1 | 0.023 | 0.39 ± 0.33 | 0.12 ± 0.10 | 0.04 ± 0.03 | |
| WRAY 15-788 | 42.2 ± 0.9 | 77.7 ± 0.4 | 0.022 | 0.76 ± 0.65 | 0.24 ± 0.21 | 0.08 ± 0.07 |
| 67.2 ± 5.9 | 132.4 ± 3.0 | 0.032 | 1.17 ± 0.72 | 0.37 ± 0.23 | 0.12 ± 0.07 | |
Notes. The gap locations, planet semi-major axes (Rp) and aspect ratios are calculated based on the fitting procedure. Planet masses (in Jupiter masses) are computed assuming three different values of the disk viscosity parameter αvisc.
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