Table 4
Results of SD modeling.
| Debris belt | ablow (μm) | amin (μm) | q | ![$\[T_{\text {dust}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq58.png) (K) |
![$\[f_{\text {disk}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq59.png) (10−4) |
![$\[M_{\text {dust}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq60.png) (10−2 M⊕) |
|---|---|---|---|---|---|---|
| HD 105 | 0.41 | 3.55 ± 0.55 | 3.58 ± 0.05 | 46±2 | 2.95 | 4.98 |
| HD 377 | 0.40 | 1.48 ± 0.18 | 3.49 ± 0.07 | 52±6 | 4.64 | 6.31 |
| HD 9672 | 2.66 | 4.97 ± 0.56 | 3.81 ± 0.05 | 66±4 | 6.80 | 17.0 |
| HD 15115 out | 0.94 | 3.17 ± 0.46 | 3.58 ± 0.12 | 54±1 | 1.99 | 4.79 |
| HD 15115 inn | 0.94 | 3.17 ± 0.46 | 3.58 ± 0.12 | 68±1 | 3.05 | 2.04 |
| HD 16743 | 1.22 | 2.48 ± 0.14 | 3.82 ± 0.07 | 70±3 | 5.08 | 8.24 |
| HD 30447 | 0.94 | 1.75 ± 0.63 | 3.23 ± 0.30 | 49±11 | 10.5 | 47.3 |
| HD 32297 | 1.53 | 2.90 ± 1.49 | 3.60 ± 0.21 | 51±20 | 60.5 | 34.1 |
| HD 35841 | 0.65 | 2.29 ± 0.14 | 3.62 ± 0.05 | 66±3 | 16.1 | 10.1 |
| HD 39060 out | 1.64 | 2.21 ± 1.43 | 4.04 ± 0.21 | 107±7 | 11.4 | 4.16 |
| HD 39060 inn | 1.64 | 2.21 ± 1.43 | 4.04 ± 0.21 | 121±7 | 19.3 | 1.45 |
| HD 61005 | (...) | 2.03 ± 0.15 | 3.64 ± 0.05 | 59±4 | 27.8 | 15.7 |
| HD 106906 | 1.80 | 1.28 ± 0.31 | 3.76 ± 0.08 | 105±4 | 12.8 | 3.54 |
| HD 109573 | 3.51 | 4.59 ± 1.25 | 3.81 ± 0.05 | 96±10 | 45.5 | 21.6 |
| HD 110058 | 1.55 | 1.82 ± 0.56 | 3.67 ± 0.16 | 107±2 | 26.1 | 5.50 |
| HD 111520 | 0.70 | 1.60 ± 0.47 | 3.54 ± 0.05 | 73±6 | 21.7 | 20.3 |
| HD 112810 | 0.87 | 3.23 ± 0.17 | 3.76 ± 0.05 | 59±3 | 10.4 | 15.8 |
| HD 114082 | 1.02 | 0.98 ± 0.15 | 3.60 ± 0.05 | 111±4 | 36.3 | 4.46 |
| HD 115600 | 1.13 | 1.86 ± 0.88 | 3.71 ± 0.30 | 115±6 | 19.9 | 1.60 |
| HD 117214 | 1.50 | 1.87 ± 095 | 3.64 ± 0.07 | 121±8 | 23.6 | 4.30 |
| HD 120326 out | 1.10 | 0.84 ± 0.29 | 3.75 ± 0.16 | 96±7 | 5.30 | 4.61 |
| HD 120326 inn | 1.10 | 0.84 ± 0.29 | 3.75 ± 0.16 | 121±7 | 12.60 | 0.81 |
| HD 121617 | 2.03 | 3.37 ± 1.47 | 3.88 ± 0.13 | 87±15 | 43.6 | 11.2 |
| HD 129590 out | 1.03 | 1.45 ± 0.47 | 3.66 ± 0.19 | 76±6 | 24.00 | 19.45 |
| HD 129590 inn | 1.03 | 1.45 ± 0.47 | 3.66 ± 0.19 | 85±6 | 40.30 | 6.95 |
| HD 131488 | 1.90 | 2.57 ± 1.32 | 3.24 ± 0.07 | 60±8 | 18.3 | 95.8 |
| HD 131835 out | 1.65 | 1.64 ± 1.05 | 3.59 ± 0.11 | 76±5 | 14.7 | 27.35 |
| HD 131835 inn | 1.65 | 1.64 ± 1.05 | 3.59 ± 0.11 | 85±5 | 22.1 | 12.18 |
| HD 141943 out | 0.71 | 0.85 ± 0.53 | 3.45 ± 0.15 | 54±6 | 1.1 | 1.64 |
| HD 141943 inn | 0.71 | 0.85 ± 0.53 | 3.45 ± 0.15 | 60±6 | 1.3 | 1.07 |
| HD 145560 | 0.76 | 2.05 ± 1.40 | 3.61 ± 0.05 | 66±6 | 30.3 | 35.5 |
| HD 146181 | 0.67 | 1.15 ± 0.24 | 3.60 ± 0.07 | 76±5 | 24.6 | 21.6 |
| HD 172555 | 1.47 | 1.73 ± 1.24 | 3.94 ± 0.38 | 207±35 | 3.50 | 0.04 |
| HD 181327 | 0.79 | 1.00 ± 0.18 | 3.42 ± 0.06 | 62±5 | 25.3 | 39.5 |
| HD 191089 | 0.76 | 1.14 ± 0.20 | 3.54 ± 0.07 | 88±5 | 15.1 | 4.64 |
| HD 107146 out(a) | 0.34 | 2.79 ± 1.17 | 3.42 ± 0.04 | 34±2 | 3.33 | 17.30 |
| HD 107146 inn(a) | 0.34 | 2.79 ± 1.17 | 3.42 ± 0.04 | 54±2 | 8.01 | 7.21 |
Notes. (a)The planetesimal belts around HD 107146 were not resolved with SPHERE. The SD modeling for this target was conducted for comparison purposes. The columns list target IDs, blowout grain sizes (ablow), minimum grain sizes (amin), the SD power-law index (q), the BB temperature corresponding to the peak of the fitted emission (![$\[T_{\text {dust}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq61.png)
), the disk IR excess (![$\[f_{\text {disk}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq62.png)
), and the belt dust masses (![$\[M_{\text {dust}}^{S ~D}\]$](/articles/aa/full_html/2025/12/aa54953-25/aa54953-25-eq63.png)
) derived from the SED fits using the SD model.
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