Table 2
Molecular line and continuum observations used in this work.
| Disk | Transition | Int. flux(1) (Jy km s−1) | Channel width (km s−1) | Channel rms (mJybeam−1) | Beam | MRS(2) | Robust | Project code | PI |
|---|---|---|---|---|---|---|---|---|---|
| LkCa15 | 12CO J = 2–1 | 16 ± 2 | 0.04 | 8.9 | 0″.34 × 0″.25 (−9.7°) | 3″.7 | −2.0 | 2018.1.01255.S | M. Benisty |
| 13CO J = 2–1 | 1.4 ± 0.2 | 0.17 | 4.4 | 0″,17 × 0″.13 (−13.7°) | 0″.5 | nat.(4) | 2018.1.00945.S | C. Qi | |
| 13CO J = 2–1 | 5.8 ± 0.6 | 0.33 | 3.1 | 0″.35 × 0″.25 (26.6°) | 4″.0 | −2.0 | 2018.1.00945.S | C. Qi | |
| 13CO J = 6–5 | 7.5 ± 0.8 | 0.5 | 2.8 | 0″.08 × 0″.05 (−18.6°) | 1″.2 | 0.5(5) | 2017.1.00727.S | J. Szulágyi | |
| 13CO J = 6–5 | 8.2 ± 0.9 | 0.44 | 25 | 0″.32 × 0″.30 (−31.2°) | 2″.1 | 0.5 | 2017.1.00727.S | J. Szulágyi | |
| C18O J = 2–1 | 1.0 ± 0.1 | 0.33 | 3.9 | 0″.36 × 0″.27 (26.6°) | 4″.0 | −2.0 | 2018.1.00945.S | C. Qi | |
| 0.45 mm cont. | 0.16 | 0″.071 × 0″.048 (−23.5°) | 1″.2 | 0.5 | 2017.1.00727.S | J. Szulágyi | |||
| HD 169142 | 12CO J = 2–1 | 9.3 ± 0.9 | 0.17 | 1.7 | 0″.05 × 0″.029 (78.8°) | 0″.6 | 0.5 | 2016.1.00344.S | S. Pérez(3) |
| 13CO J = 2–1 | 4.3 ± 0.4 | 0.17 | 2.3 | 0″.054 × 0″.035 (78.4°) | 0″.6 | 0.5 | 2016.1.00344.S | S. Pérez(3) | |
| 13CO J = 6–5 | 6.1 ± 0.7 | 0.44 | 12 | 0″.055 × 0″.054 (86.2°) | 0″.6 | 0.0 | 2017.1.00727.S | J. Szulágyi | |
| C18O J = 2–1 | 2.0 ± 0.2 | 0.17 | 1.4 | 0″.052 × 0″.031 (78.6°) | 0″.6 | 0.5 | 2016.1.00344.S | S. Pérez(3) | |
| 0.45 mm cont. | 0.52 | 0″.038 × 0″.037 (−72.0°) | 0″.6 | 0.5(6) | 2017.1.00727.S | J. Szulágyi | |||
| 1.3 mm cont. | 0.022 | 0″.036 × 0″.018(73.0°) | 0″.6 | −0.5 | 2016.1.00344.S | S. Pérez(3) |
Notes. (1)Disk integrated flux calculated from the region within the Keplerian mask. The error includes the 10% absolute flux calibration error but not any uncertainty due to resolved-out large-scale emission. (2)The maximum recoverable scale (MRS) is estimated as ~0.983λ/L5, with λ the wavelength and L5 the fifth percentile baseline of the configuration. (3)Data first presented by Pérez et al. (2019).(4)Natural weighting with a 0″.15 uv taper.(5) ALMA image for which high and intermediate spatial resolution ALMA data are combined. (6)Product data.
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