Table C.1
Disc parameters of the ARKS disc sample employed in this work.
| i[°] | PA[°] | r [au] | ∆r [au] | M* [M⊙] | d[pc] | L* [L⊙] | V* [m s−1] | Ref. | |
|---|---|---|---|---|---|---|---|---|---|
| HD 9672 | 78.7 ± 0.2 | 107.9 ± 0.2 | 135.2 ± 1.9 | 158±3 | 2.00 | 57.2 | 15 | 11906 ± 1 | 1 |
| HD 32297 | 88.3 ± 0.0 | 47.5 ± 0.0 | 115.9 ± 0.3 | 37 ± 1 | 1.57 | 130 | 7.0 |  |
1 |
| HD 121617 | 44.1 ± 0.6 | 58.7 ± 0.7 | 76.3 ± 0.4 | 18±1 | 1.90 | 118 | 14.9 |  |
1 |
| HD 131488 | 85.0 ± 0.1 | 97.2 ± 0.0 | 89.7 ± 0.1 | 13±1 | 1.80 | 152 | 12 |  |
1 |
| HD 131835 | 74.2 ± 0.2 | 59.2 ± 0.2 | 77.1 ± 0.5 | 65 ± 2 | 1.70 | 130 | 9.5 |  |
1 |
| HD 10647 | 77.8 ± 0.1 | 57.3 ± 0.3 | 103.6 ± 0.4 | 65 ± 2 | 1.12 | 17.3 | 1.6 | 27600 ± 100 | 2 |
| HD 14055 | 80.7 ± 0.2 | 162.2 ± 0.3 | 169.4 ± 2.9 | 162±9 | 2.19 | 35.7 | 29 | 5100 ± 1700 | 2 |
| HD 15115 | 86.7 ± 0.0 | 98.5 ± 0.0 | 80.7 ± 0.3 | 14±1 | 1.43 | 48.8 | 3.7 | 6900 ± 300 | 2 |
| HD 15257 | 59.4 ± 4.9 | 47.3 ± 5.5 | 184.2 ± 20.2 | 261 ± 41 | 1.75 | 49.0 | 14 | −24800 ± 2800 | 3 |
| HD 61005 | 85.9 ± 0.1 | 70.4 ± 0.1 | 72.4 ± 0.2 | 36±1 | 0.95 | 36.5 | 0.62 | 22300 ±100 | 2 |
| HD 76582 | 72.6 ± 0.7 | 104.7 ± 0.7 | 203.6 ± 4.9 | 176±9 | 1.61 | 48.9 | 9.9 | −1700 ± 200 | 2 |
| HD 84870 | 47.1 ± 2.6 | −25.7 ± 4.1 | 199.3 ± 7.8 | 232 ± 15 | 1.66 | 88.8 | 7.9 | 500 ± 200 | 2 |
| HD 95086 | 31.6 ± 3.5 | 100 ± 5.7 | 197.0 ± 4.6 | 173±8 | 1.54 | 86.5 | 6.4 | 18000 ± 200 | 2 |
| HD 109573 | 76.6 ± 0.1 | 26.5 ± 0.0 | 75.9 ± 0.1 | 7±0 | 2.14 | 70.8 | 25 | 10900 ± 600 | 2 |
| HD 145560 | 47.6 ± 0.6 | 39.4 ± 0.9 | 75.4 ± 0.5 | 29 ± 2 | 1.35 | 121 | 3.3 | 2800 ± 500 | 2 |
| HD 161868 | 66.1 ± 1.5 | 57.6 ± 1.6 | 121.2 ± 3.7 | 134±8 | 2.11 | 29.7 | 24 | −12300±500 | 2 |
| HD 170773 | 32.9 ± 1.9 | 113.0 ± 2.9 | 191.9 ± 2.9 | 66 ± 4 | 1.4 | 36.9 | 3.6 | −17700±200 | 2 |
| TYC 9340-437-1 | 18.0 ± 8.0 | 149.2 ± 20.2 | 95.7 ± 2.5 | 99 ± 5 | 0.75 | 36.7 | 0.19 | 7980 ± 20 | 4 |
Notes. The inclination, PA, disc radius (r) and disc width (Δr) (2nd, 3rd, 4th and 5th columns) are the best fit parameters derived from MCMC sampling carried out by Marino et al. (2026b). The listed values correspond to the median and the 16th and 84th percentiles to estimate the uncertainties. For sources with a double Gaussian (HD 107146, HD 92945 and HD 15115), r represents the average between the two Gaussian centres and Δr is the sum of the FWHM of the two Gaussians. Stellar masses in the 6th column were estimated as described in Appendix A in Marino et al. (2026b). The 7th column indicates the distance according to Gaia DR3 (Gaia Collaboration 2023). The stellar luminosity (8th column) were taken from Matrà et al. (2025). The 9th column indicates the stellar barycentric radial velocity. V* for gas-bearing systems were measured by fitting a Gaussian to the discs spectro-spatailly stacked spectra, while V* for gas-free systems were taken from the literature; the corresponding reference is listed in the 10th column.
Velocity references. 1. This work, 2. Gaia Collaboration (2023), 3. Gontcharov (2006), 4. Zúñiga-Fernández et al. (2021)
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