Table F.2
Disk properties derived from the fit to the emission using a 2D Gaussian fit.
| source | λ (mm) | Fν (mJy) | Deconv. major FWHM (au) | Deconv. minor FWHM (au) | R95 (au) | R68 (au) |
|---|---|---|---|---|---|---|
| RCrA IRS7B b | 1.3 | 35.64 ± 0.68 | 27.54 ± 0.55 | 11.7 ± 0.30 | 28.65 ± 0.57 | 17.66 ± 0.35 |
| 3 | 6.32 ± 0.16 | 25.37 ± 0.67 | 10.4 ± 0.34 | 26.40 ± 0.70 | 16.27 ± 0.43 | |
| RCrA IRS7A | 1.3 | 12.32 ± 0.24 | 7.02 ± 0.30 | 3.9 ± 0.21 | 7.30 ± 0.31 | 4.50 ± 0.19 |
| 3a | 6.54 ± 0.25 | 10.07 ± 0.49 | 6.1 ± 0.48 | 10.48 ± 0.51 | 6.46 ± 0.32 | |
| CrA24 | 3 | 1.82 ± 0.09 | 16.21 ± 0.92 | 4.8 ± 0.54 | 16.87 ± 0.96 | 10.40 ± 0.59 |
| CXO 34 | 1.3 | 16.27 ± 0.2 | 18.53 ± 0.27 | 7.7 ± 0.11 | 19.28 ± 0.28 | 11.88 ± 0.17 |
| 3 | 3.62 ± 0.04 | 17.60 ± 0.23 | 7.6 ± 0.14 | 18.31 ± 0.24 | 11.28 ± 0.15 | |
| Elias 29 | 1.3 | 13.93 ± 0.04 | 2.07 ± 0.04 | 1.8 ± 0.04 | 2.15 ± 0.04 | 1.33 ± 0.02 |
| 3 | 4.25 ± 0.02 | 2.23 ± 0.08 | 2.0 ± 0.08 | 2.32 ± 0.08 | 1.43 ± 0.05 | |
| RCrA SMM2 a | 3 | 0.51 ± 0.04 | point source | point source | ≲ 3b | ≲ 2b |
| RCrA SMM2 b | 3 | 0.51 ± 0.046 | point source | point source | ≲ 3 | ≲ 2 |
| VLA 1623 Aa | 1.3 | 49.85 ± 0.39 | 16.42 ± 0.14 | 9.0 ± 0.09 | 17.08 ± 0.15 | 10.53 ± 0.09 |
| 3 | 10.00 ± 0.06 | 14.32 ± 0.10 | 7.4 ± 0.09 | 14.90 ± 0.11 | 9.18 ± 0.07 | |
| VLA 1623 Ab | 1.3 | 45.61 ± 0.38 | 14.02 ± 0.10 | 7.2 ± 0.09 | 14.59 ± 0.10 | 8.99 ± 0.06 |
| 3 | 9.78 ± 0.06 | 15.84 ± 0.14 | 8.6 ± 0.10 | 16.48 ± 0.15 | 10.16 ± 0.09 | |
| IRAS 16293 A1 | 1.3 | 5.90 ± 0.5 | ... | ... | ≲ 6.5c | ≲ 4c 0.00 |
| 3 | 4.91 ± 3.6 | 4.79 ± 2.68 | 2.8 ± 2.26 | 4.99 ± 2.79 | 3.07 ± 1.72 | |
| IRAS 16293 A2 | 1.3 | 6.00 ± 0.6 | ... | ... | ≲ 12.6c | ≲ 7.8c 0.00 |
| 3 | 4.20 ± 0.1 | 10.58 ± 2.12 | 6.8 ± 3.53 | 11.00 ± 2.20 | 6.78 ± 1.36 |
Notes.a The 3 mm observations likely contain significant non-thermal emission, and thus the disk size at this wavelength is not reliable.
b The results from the fit is that the source is a point source. Upper limit corresponds to assuming the deconvolved size of the source is a third of the major beam axis. c Imfit could not deconvolve the source from the beam because it was only marginally resolved in just one direction. Values in the table are thus only provided as a reference. They are calculated assuming the deconvolved FWHM of the source is a third of the minor beam axis divided by the cosine of the inclination, the latter derived from the 3 mm observations.
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