Table D.1
Comparison of disk mass estimates from Pan & Schlichting (2012) (1) and K21 (2), as well as the assumed millimeter dust masses Mmm used in each of these models.
| Target | Mdisk [M⊕] (1) |  [M⊕] (2) |
Mmm [M⊕] (1) | Mmm [M⊕] (2) | Rescaled  [M⊕] |
Compatible? |
|---|---|---|---|---|---|---|
| HD 9672 | 86.6 | 14.3 | 4.95 × 10−1 | 2.8 × 10−1 | 25.3 | yes |
| HD 15115 | 3.72 | 7.0 | 6.17 × 10−3 | 8.5 × 10−2 | 0.51 | yes, rescaled |
| HD 39060 | 104 | 5.5 | 1.83 × 10−1 | 7.9 × 10−2 | 12.7 | yes |
| HD 61005 | 10.2 | 14.2 | 1.26 × 10−1 | 1.3 × 10−1 | 13.8 | no |
| HD 131488 | 9.01 | 85.8 | 2.75 × 10−1 | 7.2 × 10−1 | 32.8 | no |
| HD 131835 | 49.7 | 39.1 | 4.08 × 10−1 | 3.8 × 10−1 | 42.0 | yes |
| HD 197481 | 0.830 | 1.8 | 1.49 × 10−2 | 1.4 × 10−2 | 1.92 | no |
Notes. We rescale the originally reported 
to use the Mmm obtained from our fiducial models. The rescaled 
are compatible with the Mdisk obtained from the Pan & Schlichting (2012) model for HD 9672, HD 15115, HD 39060, and HD 131835, and incompatible for HD 61005, HD 131488, and HD 197481. These discrepancies may stem from differences in model assumptions (see Sect. 5.2). For the Pan & Schlichting (2012) model, difficulties constraining the scale height aspect ratio (which sets model parameter ⟨vrel⟩) may also contribute, particularly for HD 131488 and HD 197481 which are both noted to have h measurements limited by the resolution of the observations.
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