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Table A.1

Datasets and corresponding parameters for each Herbig disk. The rms noise is for a line-free channel at the given velocity resolution. When the CO isotopologue observations are coming from different projects, multiple project codes are listed.

12CO 13CO C18O

name Spat.res. (″) Vel.res. (km s−1) rms (mJy beam−1) Spat.res. (″) Vel.res. (km s−1) rms (mJy beam−1) Spat.res. (″) Vel.res. (km s−1 ) rms (mJy beam−1) Project codes
AB Aur 0.39 × 0.28 (10°) 0.20 16.83 2012.1.00303.S*
1.14 × 0.70 (14°) 0.20 5.67 1.14 × 0.71 (13°) 0.20 4.57 2019.1.00579.S
AK Sco 0.15 × 0.11 (−63°) 1.00 1.35 0.16 × 0.12 (−63°) 1.00 1.53 0.16 × 0.13 (−75°) 1.00 0.95 2016.1.00204.S
CQ Tau 0.11 × 0.08 (18°) 0.32 1.53 0.12 × 0.09 (26°) 0.66 1.32 0.12 × 0.09 (25°) 0.67 0.91 2017.1.01404.S
HD 100453 0.29 × 0.21 (40°) 0.20 3.26 0.31 × 0.23 (39°) 0.20 2.74 0.30 × 0.22 (38°) 0.20 2.05 2015.1.00192.S
HD 100546 0.27 × 0.17 (−85°) 0.20 3.65 0.27 × 0.19 (−10°) 0.20 3.44 0.27 × 0.19 (−10°) 0.20 2.61 2016.1.00344.S
HD 104237 0.31 × 0.22 (−12°) 0.70 3.28 0.32 × 0.22 (−14°) 0.70 2.43 0.32 × 0.22 (−13°) 0.70 1.92 2017.1.01419.S
HD 135344B 0.34 × 0.30 (75°) 0.20 7.64 0.35 × 0.30 (84°) 0.20 10.43 2012.1.00158.S*
0.36 × 0.29 (−68°) 0.20 11.79 2012.1.00870.S
HD 139614 0.79 × 0.60 (−49°) 0.40 12.13 0.81 × 0.60 (−47°) 0.40 8.03 2015.1.01600.S
HD 141569 0.41 × 0.33 (−61°) 0.42 5.99 2012.1.00698.S*
0.76 × 0.66 (82°) 0.40 15.19 0.72 × 0.67 (−66°) 0.40 10.91 2015.1.01600.S
HD 142527 0.93 × 0.81 (−85°) 0.20 6.35 0.97 × 0.84 (−87°) 0.20 6.68 0.98 × 0.85 (−88°) 0.20 4.92 2015.1.01353.S
HD 142666 1.05 × 0.82 (87°) 0.20 16.18 1.04 × 0.85 (87°) 0.20 10.46 2015.1.01600.S
0.21 × 0.20 (−70°) 0.32 2.27 2016.1.00484.L
HD 163296 0.65 × 0.56 (71°) 0.20 3.63 0.68 × 0.59 (68°) 0.20 2.98 0.69 × 0.59 (72°) 0.20 2.11 2018.1.01055.L
HD 169142 0.37 × 0.31 (−77°) 0.20 3.61 0.39 × 0.33 (88°) 0.20 3.67 0.39 × 0.33 (−85°) 0.20 2.64 2016.1.00344.S
HD 176386 0.40 × 0.30 (77°) 0.30 17.88 0.42 × 0.31 (79°) 0.30 17.33 0.42 × 0.31 (78°) 0.30 14.01 2015.1.01058.S
HD 245185 0.42 × 0.39 (−85°) 0.70 8.05 2017.1.00466.S
HD 290764 0.08 × 0.07 (−80°) 1.00 2.04 2015.1.00986.S*
0.21 × 0.14 (−62°) 1.00 1.60 0.23 × 0.14 (−63°) 1.00 2.06 2017.1.01607.S*
HD 31648 1.16 × 0.88 (15°) 0.20 7.35 1.22 × 0.92 (13°) 0.20 7.64 1.22 × 0.92 (14°) 0.20 5.89 2016.1.00724.S
HD 34282 0.27 × 0.24 (68°) 0.20 4.50 0.28 × 0.27 (63°) 0.20 3.32 0.28 × 0.27 (59°) 0.20 2.46 2015.1.00192.S
HD 36112 0.19 × 0.14 (−17°) 1.40 1.56 0.20 × 0.15 (−16°) 1.40 1.90 0.20 × 0.15 (−16°) 1.40 1.28 2017.1.00940.S
HD 58647 0.54 × 0.45 (73°) 0.20 6.03 0.64 × 0.54 (74°) 0.20 4.69 0.65 × 0.55 (77°) 0.20 3.87 2018.1.00814.S
HD 9672 1.70 × 1.15 (−75°) 0.64 3.61 1.75 × 1.25 (−75°) 0.66 3.92 1.78 × 1.20 (−74°) 0.67 2.93 2018.1.01222.S
HD 97048 1.22 × 0.76 (−31°) 0.30 7.81 1.30 × 0.79 (−32°) 0.30 7.17 1.31 × 0.80 (−31°) 0.30 5.89 2015.1.00192.S
HR 5999 0.28 × 0.27 (87°) 0.40 12.62 0.29 × 0.29 (−82°) 0.40 12.86 0.29 × 0.29 (−74°) 0.40 9.57 2015.1.00222.S
KK Oph 0.77 × 0.68 (73°) 0.40 28.90 0.68 × 0.63 (−61°) 0.40 11.98 2015.1.01600.S
MWC 297 0.41 × 0.36 (71°) 0.20 7.29 0.43 × 0.38 (74°) 0.20 5.83 0.43 × 0.38 (75°) 0.20 4.65 2018.1.00814.S
TY CrA 0.40 × 0.30 (78°) 0.30 17.60 0.42 × 0.31 (78°) 0.30 17.60 0.42 × 0.31 (77°) 0.30 13.67 2015.1.01058.S
V718 Sco 1.01 × 0.82 (−67°) 0.40 10.52 0.99 × 0.85 (−63°) 0.40 8.00 2015.1.01600.S
V892 Tau 0.26 × 0.19 (4°) 0.32 21.12 0.27 × 0.19 (4°) 0.66 5.57 0.28 × 0.20 (5°) 0.67 3.93 2013.1.00498.S
VV Ser 1.73 × 1.21 (−63°) 0.40 34.83 2019.1.00218.S
Z CMa 0.22 × 0.20 (−78°) 0.20 5.55 0.23 × 0.21 (−79°) 0.20 6.15 0.23 × 0.21 (−76°) 0.20 4.68 2016.1.00110.S
BH Cep 1.10 × 0.82 (31°) 0.40 9.42 1.11 × 0.82 (32°) 0.40 9.61 S21 AS
BO Cep 1.03 × 0.85 (64°) 0.40 11.31 1.04 × 0.85 (61°) 0.40 10.77 S21 AS
HD 200775 1.09 × 0.85 (51°) 0.40 11.47 1.09 × 0.86 (51°) 0.40 11.24 S21 AS
SV Cep 1.01 × 0.83 (71°) 0.40 10.83 1.01 × 0.84 (70°) 0.40 10.69 S21 AS
XY Per 1.09 × 0.66 (8°) 0.40 10.33 1.10 × 0.66 (8°) 0.40 10.44 S21 AS

Notes. The Project codes with an asterisk are for the J = 3−2 transition, all others are for the J = 2−1 transition.

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