Table B.1
Continuum best-fit parameters
| Name | R [au] | ∆R [au] | h | i [°] | PA [°] | Mdust [M⊕] | F* [μJy] | ∆RA [mas] | ∆Dec [mas] |
|---|---|---|---|---|---|---|---|---|---|
| HD 9672g | 135.2 ± 1.9 | 158±3 | 0.066 ± 0.004 | 78.7 ± 0.2 | 107.9 ± 0.2 | 0.21 | < 19 (28) | 68 ± 76 | −33 ± 30 |
| HD 10647 | 103.6 ± 0.4 | 65 ± 2 | 0.062 ± 0.003 | 77.8 ± 0.1 | 57.3 ± 0.1 | 0.03 | 131 ± 9 (96) | 90 ± 56 | 28 ± 51 |
| HD 14055 | 169.4 ± 2.9 | 162±9 | 0.048 ± 0.007 | 80.7 ± 0.2 | 162.2 ± 0.3 | 0.05 | 87 ± 11 (111) | −57 ± 59 | −84±155 |
| HD 15115 | 80.7 ± 0.3 | 14±1 | 0.017 ± 0.001 | 86.7 ± 0.0 | 98.5 ± 0.0 | 0.07 | 24 ± 4 (22) | 44 ± 12 | −8 ± 5 |
| HD 15257 | 184.2 ± 20.2 | 261 ± 41 | 59.4 ± 4.9 | 47.3 ± 5.5 | 0.06 | 79 ± 35m (73) | 86 ± 134 | 14 ± 180 | |
| HD 32297g | 115.9 ± 0.3 | 37 ± 1 | 0.011 ± 0.001 | 88.3 ± 0.0 | 47.5 ± 0.0 | 0.87 | 24 ± 13m (3) | 19±4 | 18±4 |
| HD 39060g | 104.3 ± 1.4 | 97 ± 3 | 0.059 ± 0.003 | 86.4 ± 0.2 | 29.9 ± 0.1 | 0.12 | 86 ± 14 (70) | −54 ± 14 | −2 ± 20 |
| HD 61005 | 72.4 ± 0.2 | 36±1 | 0.020 ± 0.002 | 85.9 ± 0.1 | 70.4 ± 0.1 | 0.15 | (12) | 8 ± 22 | −4 ± 8 |
| HD 76582 | 203.6 ± 4.9 | 176±9 | 72.6 ± 0.7 | 104.7 ± 0.7 | 0.12 | (37) | 100 ± 46 | 54 ± 33 | |
| HD 84870 | 199.3 ± 7.8 | 232 ± 15 | 47.1 ± 2.6 | −25.7 ± 4.1 | 0.13 | (9) | 81 ± 57 | −103±63 | |
| HD 92945 | 78.2 ± 1.0 | 73 ± 6 | 0.032 ± 0.013m | 65.4 ± 0.6 | 100.0 ± 0.6 | 0.06 | 45 ± 13 (25) | −84 ± 55 | 12 ± 35 |
| HD 95086 | 197.0 ± 4.6 | 173±8 | 31.6 ± 3.5 | 100.0 ± 5.7 | 0.49 | (9) | −91 ± 45 | 127 ± 34 | |
| HD 107146 | 84.2 ± 0.2 | 89±1 | 19.3 ± 0.6 | 153.2 ± 1.7 | 0.22 | (29) | 36 ± 35 | −48 ± 35 | |
| HD 109573 | 75.9 ± 0.1 | 7±0 | < 0.02 | 76.6 ± 0.1 | 26.5 ± 0.0 | 0.23 | (20) | 11 ± 2 | −32±2 |
| HD 121617g | 76.3 ± 0.4 | 18±1 | 44.1 ± 0.6 | 58.7 ± 0.7 | 0.21 | (6) | 8±8 | 14±7 | |
| HD 131488g | 89.7 ± 0.1 | 13±1 | 0.011 ± 0.001 | 85.0 ± 0.1 | 97.2 ± 0.0 | 0.58 | (3) | 0±2 | 1±1 |
| HD 131835g | 77.1 ± 0.5 | 65 ± 2 | 0.049 ± 0.005 | 74.2 ± 0.2 | 59.2 ± 0.2 | 0.45 | (5) | 6±6 | 3±6 |
| HD 145560 | 75.4 ± 0.5 | 29 ± 2 | < 0.11 | 47.6 ± 0.6 | 39.4 ± 0.9 | 0.28 | (4) | 15±12 | −9 ± 11 |
| HD 161868 | 121.2 ± 3.7 | 134±8 | 66.1 ± 1.5 | 57.6 ± 1.6 | 0.03 | 161 ± 18 (146) | 49 ± 40 | −131±42 | |
| HD 170773 | 191.9 ± 2.6 | 66 ± 4 | 32.9 ± 1.9 | 113.0 ± 2.9 | 0.16 | 84 ± 21 (39) | −77 ± 40 | 26 ± 35 | |
| HD 197481 | 33.6 ± 0.2 | 13±1 | 0.015 ± 0.003 | 88.3 ± 0.1 | 128.6 ± 0.1 | 0.012 | 245 ± 14 (50) | 32 ± 15 | 6±13 |
| HD 206893 | 105.1 ± 6.0 | 116 ± 10 | 45.2 ± 2.5 | 60.3 ± 3.6 | 0.04 | (12) | 40 ± 132 | 53 ± 106 | |
| TYC 9340-437-1 | 95.7 ± 2.5 | 99 ± 5 | 18.0 ± 8.0 | 149.2 ± 20.2 | 0.17 | (10) | 81 ± 65 | −98 ± 64 | |
| HD 218396 | 240.4 ± 4.6 | 182±9 | 28.8 ± 3.3 | 49.7 ± 5.7 | 0.11 | 59 ± 10 (35) | −41 ± 65 | −57 ± 69 |
Notes. Best-fit parameters derived from the MCMC sampling, using the median and the 16th and 84th percentiles to estimate the uncertainties. For sources fitted with a double Gaussian (HD 107146, HD 92945, and HD 15115), R represents the average between the two Gaussian centres and ∆R is the sum of the FWHMs of the two Gaussians. Column 8 shows the stellar flux at the shortest available ALMA wavelength as derived from the MCMC if it was included as a free parameter and the photospheric flux expected from extrapolating the stellar SED in brackets. For marginalised distributions of h and F* peaking at zero, we present upper limits estimated with the 99.7 percentile. If their marginalised distributions peaked above zero but still extended to zero, we flagged those marginal values ‘m’. The last two columns show the best-fit right ascension and declination offsets for the long baseline execution used as a reference. Systems with CO gas are flagged ‘g’
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