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Table A.2

Continuum and CO line (J = 2 − 1 or J = 3 − 2) fluxes as well as dust and gas radii.

Continuum 12CO 13CO C 18O

Name Flux Rdust, 68% Rdust, 90% Flux Rgas, 68% Rgas, 90% Flux Rgas, 68% Rgas, 90% Flux Rgas, 68% Rgas, 90% Mdust Log10(Mgas)
(mJy) (au) (au) (Jy km s−1 ) (au) (au) (Jy km s−1) (au) (au) (Jy km s−1) (au) (au) (M) (M)
AK Sco 26.14 42±2 53±2 2.18±0.05 78±4 114±5 0.68±0.04 66±6 97±18 0.27±0.02 52±5 69±11 6.0±0.6 −2.6±1.2
Ass ChaT2-21 <1.21* <0.29* <0.1
Ass ChaT2-54 <3.16* <0.89* <5.06* <5.20* <0.5
BE Ori 0.94 <286 <373 <0.33 <0.39 <0.31 l.7±0.2
Brun 656 <1.68 <3.0
CO Ori <7.78 <2.09 <2.51 <1.85 <10.7
CR Cha 139.47 63±3 88±3 2.22±0.04 158±27 249±27 0.74±0.05 150±28 233±111 0.29±0.02 139±28 201±28 69.7±7.0 −1.7±0.8
CV Cha 56.70* <76 <119 <4.99 * <4.51* 10.4±1.0
DI Cha 23.76* <73 <100 <4.48* <1.80* 3.4±0.3
GW Ori 200.37 286±12 381±12 51.09±0.06 778±16 1032±16 6.28±0.07 576±16 805±20 l.30±0.03 418±16 559±20 241.9±27.3 −1.1±0.4
Haro 1-6 3.22 <108 <155 <0.88 <0.99 <0.44 0.6±0.1
HBC 442 <9.29 <2.41 <2.58 <2.42 <16.2
HBC 502 <4.57 <7.9
HD 34700 10.51 <189 <244 6.65±0.06 301±38 421±38 <1.20 <0.91 10.7±1.1
HD 35929 0.22 <12 <17 <0.04 <0.04 <0.03 0.23±0.03
HD 135344B 539.69* 81±10 109±10 20.07±0.18* 158±10 219±10 8.86±0.08* 119±9 171 ±9 3.55±0.08* 86±9 125±9 35.8±3.7 −1.7±0.4
HD 142527 1048.15 208±9 236±9 27.14±0.10 542±30 793±30 11.88±1.07 334±31 491±31 3.91 ±0.04 271 ±31 368±31 231.2±23.4 −0.8±0.2
HD 142666 118.55 40±1 52±1 4.05±0.03 136±6 186±6 1.51±0.06 <182 <260 0.64±0.04 <164 <236 26.0±2.6 −1.5±0.7
HD 144432 44.92 <587 <856 <2.25 <1.59 <1.21 13.1±1.3
HD 288313 1.03 <99 <166 <0.15 <0.18 <0.16 1.6±0.2
HD 294260 41.53 <123 <181 l.72±0.03 <233 <348 74.4±7.9
HQ Tau 3.94 <22 <30 <0.18 <0.13 1.6±0.2
HT Lup 62.54 19±1 25±1 4.78±0.04 111±2 141 ±2 <0.24 <0.18 18.0±1.8
LkHA 310 14.55 <109 <157 <0.18 <0.16 <0.15 36.7±4.2
LkHA 330 52.33 123±5 141 ±5 2.00 ± 0.12 219±23 337±54 l.48±0.08 194±14 261 ±29 0.63±0.04 117±7 143±12 47.2±5.3 −1.2±0.5
PDS 156 9.94 <90 <129 0.35±0.03 <164 <273 <0.06 <0.05 16.2±1.7
PDS 277 39.48 <114 <168 0.62±0.04 <217 <322 <0.72 <0.67 48.8±5.0
PR Ori 21.82 <344 <510 41.7±4.3
RY Ori <22.49 <2.58 <2.50 <2.16 <40.0
RY Tau 207.91 51±1 65±1 7.89±0.20 171 ±7 237±10 l.85±0.09 114±7 156±14 0.46±0.05 86±10 112±21 37.1±23.9 –3.3±0.4
SR 21 88.20 61 ±3 69±3 0.53±0.02 28±4 35±4 0.50±0.02 31±4 42±4 0.38±0.02 34±4 47±4 23.8±2.4 –1.2±0.6
SU Aur 16.73 <58 <100 13.52±0.13 255±11 346±11 0.91±0.13 211 ±65 320±l41 4.9±0.5
SW Ori 7.46 <285 <396 <0.38 <0.44 <0.34 15.7±1.6
T Tau 171.62 16±1 22±1 47.3±4.8
UX Tau 64.54 49±7 64±7 8.46±0.12 216±9 453±24 2.10±0.06 94±9 152±13 0.96±0.04 82±9 132±20 13.7±1.4 −1.4±0.6

Notes. For AK Sco, HD 135344B, HD 142526, and HD 142666 the fluxes, radii, and gas masses were taken from Stapper et al. (2022) and Stapper et al. (2024). The dust masses were recalculated using the stellar luminosities of Valegård et al. (2021). All fluxes with an asterisk are for the J = 3 − 2 transition, the other fluxes are for the 7 = 2-1 transition. A non-detection is indicated by a dash. On all fluxes there is an additional 10% calibration error.

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