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Table D.1

12CO and continuum emission used to plot Figs. 7a and b.

ID Name CO J = 2 → 1 Continuum CO J = 3 → 2 Continuum References
(Jy km s-1) 1.3 mm (mJy) (Jy km s-1) 0.8 mm (mJy)
1 CIDA 1 0.9 ± 0.8 16 ± 8 1.45 ± 0.05 27 ± 3 1
2 †IRAS 04113+2758 10 ± 12 196 ± 96 19.1 410 ± 5 2
3 CY Tau 2.02 ± 0.08 111 ± 3 3.6 ± 1.0 140 ± 5 3, 4, 5
4 †FQ Tau 0.2 ± 0.2 6 ± 3 0.239 8.8 ± 1.2 2
5 BP Tau 1.11 ± 0.08 58.2 ± 1.3 1.90 ± 0.59 130 ± 7 3, 4, 5
6 RY Tau 6.6 229 ± 17 123 ± 37 560 ± 30 6, 7, 8, 5
7 †FV Tau A 1.3 ± 1.5 6.17 ± 0.16 2.17 31 ± 1.4 9, 2
8 †FW Tau c 0.156 3.4 ± 0.2 0.2 ± 0.1 4.9 ± 2.4 51
9 †FX Tau 0.9 ± 1.0 7.1 ± 0.15 1.49 17 ± 0.9 9, 2
10 †DK Tau 0.9 ± 1.1 35 ± 7 1.56 66 ± 1.0 9, 2
11 †HK Tau A 2.3 ± 2.7 33 ± 0.15 4.1 78 ± 1.1 9, 2
12 †HK Tau B 1.9 ± 2.2 12.6 ± 0.15 3.39 57 ± 1.3 9, 2
13 †V710 Tau 1.8 ± 2.1 59.18 ± 0.33 3.23 142 ± 1.5 9, 2
14 †GG Tau 13 ± 16 546 ± 298 53 ± 15 1255 ± 57 8, 5
15 GK Tau A 2.00 ± 2.33 5.33 ± 0.56 3.56 15 ± 1 9, 2
16 DL Tau 1.98 ± 0.12 204 ± 2 3.5 ± 1.1 440 ± 40 3, 4, 10
17 †HN Tau 1.4 ± 1.7 12.8 ± 0.2 2.48 37 ± 1.1 9, 2
18 DM Tau 14.87 ± 0.12 109 ± 2.4 20 ± 6 237 ± 12 11, 4, 8, 5
19 †IT Tau B 0.6 ± 0.7 6.5 ± 3.1 1.03 10 ± 0.9 2
20 AA Tau 8.2 ± 0.16 88 ± 9 15.5 ± 4.7 144 ± 5 11, 5
21 †HO Tau 0.8 ± 0.9 17.06 ± 0.27 1.36 38 ± 1 9, 2
22 †HBC 411 B 0.4 ± 0.4 5.8 ± 0.27 0.624 14 ± 1 9, 2
23 LkCa 15 13.94 ± 0.15 110 ± 2 23 ± 7 428 ± 11 11, 4, 8, 5
24 J04442713+2512164 0.6 ± 0.6 5.9 ± 3.6 0.98 ± 0.03 9 ± 2 1
25 †DQ Tau 0.97 ± 0.11 83.1 ± 2.8 1.7 ± 0.6 161 ± 86 3, 4
26 DR Tau 49 ± 65 159 ± 11 103 ± 31 533 ± 7 5, 8
27 †DS Tau 3.7 ± 4.3 19.94 ± 0.25 6.69 43 ± 1.4 9, 2
28 GM Aur 19.41 ± 0.11 176 ± 5.3 29.0 ± 8.7 707 ± 4 11, 4, 8, 12
29 V836 Tau 0.84 ± 0.18 24 ± 2 1.42 ± 0.65 42 ± 23 13
30 †IRAS 05022+2527 2.9 ± 3.4 35.22 ± 0.26 5.21 87 ± 1.3 9, 2
31 HD 34282 4.2 ± 0.1 110 ± 10 7.7 ± 2.2 218 ± 131 2
32 HD 294268 < 0.9 5 ± 0.8 < 1.5 ± 1.8 19.4 ± 5.4 52
33 V2731 Ori 0.95 ± 0.13 10.7 ± 0.8 1.6 ± 0.6 32.6 ± 4.8 52
34 J05391573-0230568 < 2.43 8 ± 1 < 4.3 ± 1.9 13 ± 2.7 52
35 V602 Ori 0.34 ± 0.08 7.8 ± 0.8 0.5 ± 0.3 17.4 ± 4.2 52
36 V606 Ori 0.36 ± 0.07 14.3 ± 0.8 0.6 ± 0.2 31.4 ± 4.8 52
37 TWA 34 0.34 ± 0.03 0.54 ± 0.06 0.55 ± 0.17 0.66 ± 0.32 15
38 TW Hya 12.4 ± 1 540 ± 30 45 ± 4 1620 ± 50
39 T Cha 7 ± 7 81.8 12.46 ± 0.11 198 ± 4
40 HD 135344 10 ± 10 153 ± 75 18.6 ± 0.8 314 ± 4.5 16, 17
41 HD 142527 17.4 ± 0.01 1090 ± 0.3 34 ± 10 2700 ± 1500 18
42 HD 143006 4.28 ± 0.04 43 ± 3 3 ± 1 78 ± 43 19, 20, 16
43 J16042165-2130284 11 ± 11 113 ± 53 21.4 ± 0.2 226 ± 1 21
44 Sz 91 4.93 ± 0.02 40 ± 1 8.55 34.5 ± 2.9 53, 22, 23
45 †AS 205 A (N) 19.23 ± 0.27 377 ± 2 65 905 ± 7 24, 25
46 †AS 205 B (S) 3.02 ± 0.22 64 ± 1 5.4 ± 1.8 55 ± 7 24, 25
47 GSS 26 >4 176 > 7.3 ± 19.9 364 ± 267 2
48 GSS 39 >25 304 > 49.9 ± 2.1 663 ± 3 2, 25
49 WL 18 >0.3 24 > 0.5 ± 1.7 42 ± 28 2
50 WL 14 >0.2 <0.2 > 0.3 ± 1.7 < 0.2 ± 1.2 2
51 ISO-Oph 102 0.3 ± 0.3 2.9 ± 1.2 0.53 ± 0.05 4.1 ± 0.2 26
52 YLW 16c >1.6 45 > 2.8 ± 1.8 82 ± 58 2
53 ROX 25 >0.6 29 > 1.0 ± 1.7 51 ± 35 2
54 Flying Saucer >2.1 32 > 3.7 ± 1.9 57 ± 39 2
55 AS 209 7.4 300 16.5 577 ± 3
56 †V4046 Sgr 11.38 ± 0.16 451 ± 20 22 ± 7 1020 ± 600 27, 28
Herbig AeBe disks
57 †V892 Tau 22 ± 29 293 ± 167 85.4 ± 26 638 ± 54 8, 5
58 AB Aur 801 103 ± 18 153 ± 4 359 ± 67 2, 5, 16
59 MWC 480 22 ± 0.2 289.3 ± 2.5 52 ± 1.1 626 ± 336 11, 4, 16
60 MWC 758 7.9 ± 8.9 56 ± 1 15 ± 2 217 ± 40 29, 16, 30
61 HD 245185 0.17 ± 0.03 29 ± 6 0.3 ± 0.1 74.1 ± 4.2 14
62 CQ Tau 3.1 ± 0.18 162 ± 2 5.95 ± 0.96 421 ± 9 11, 4, 16, 31
63 HD 100546 49 ± 62 540 ± 272 158 ± 24 1240 32, 33
64 †AK Sco 2.21 ± 0.01 32.65 ± 0.07 5.7 ± 1.9 52 ± 38 34
65 HD 163296 46 ± 5 705 ± 12 109 ± 11 1910 ± 20 35, 36
66 HD 169142 2.72 ± 0.7 169 ± 5 32.6 ± 2.5 349 ± 190 37, 16
WTTS disks
67 J04182147+1658470 <0.09 <0.436 < 0.14 < 0.53 38
68 †J04192625+2826142 <0.09 0.533 < 0.14 0.66 ± 0.38 38
69 J04242321+2650084 <0.09 <0.426 < 0.14 < 0.51 38
70 J04314503+2859081 <0.09 <0.435 < 0.14 < 0.53 38
71 J04325323+1735337 <0.09 <0.438 < 0.14 < 0.53 38
72 J04330422+2921499 <0.09 <0.431 < 0.14 < 0.52 38
73 J04364912+2412588 <0.09 <0.435 < 0.14 < 0.53 38
74 J04403979+2519061 <0.09 <0.431 < 0.14 < 0.52 38
75 †J04420548+2522562 <0.09 <0.423 < 0.14 < 0.51 38
76 J08413703-7903304 <0.09 <0.476 < 0.14 < 0.58 38
77 J08422372-7904030 <0.09 <0.472 < 0.14 < 0.58 38
78 J11073519-7734493 <0.09 <0.541 < 0.14 < 0.67 38
79 †J11124268-7722230 <0.09 <0.494 < 0.14 < 0.60 38
80 †J16002612-4153553 <0.09 0.696 < 0.14 0.88 ± 0.5 38
81 J16010896-3320141 <0.09 <0.442 < 0.14 < 0.53 38
82 J16031181-3239202 <0.09 <0.453 < 0.14 < 0.55 38
83 †J16085553-3902339 <0.09 1.813 < 0.14 2.5 ± 1.5 38
84 †J16124119-1924182 <0.09 <0.459 < 0.14 < 0.56 38
85 †J16220961-1953005 <0.09 <0.483 < 0.14 < 0.59 38
86 J16223757-2345508 <0.09 <0.461 < 0.14 < 0.56 38
87 J16251469-2456069 <0.09 <0.453 < 0.14 < 0.55 38
88 †J16275209-2440503 <0.09 <0.442 < 0.14 < 0.53 38
89 †J19002906-3656036 <0.09 0.569 < 0.14 0.7 ± 0.3 38
90 †J19012901-3701484 <0.09 <0.465 < 0.14 < 0.56 38
Hybrid disks
91 49 Ceti 2 ± 0.3 <2.1 9.5 ± 1.9 8.2 ± 1.9 39, 40
92 HD 21997 2.17 ± 0.23 < 1 2.52 ± 0.27 2.69 ± 0.3 41, 2, 42
93 HD 131835 0.798 ± 0.035 5.6 ± 4.9 2.74 ± 0.55 8.5 ± 4.4 54, 43, 44
94 HIP 76310 1,41 ± 0.08 1.2 ± 0.2 2.4 ± 0.5 1.6 ± 1.1 54
95 HD 141569 9.57 ± 0.03 3.7 ± 0.4 14.6 ± 1 5.3 ± 0.6 45, 16, 46
96 HIP 84881 1.18 ± 0.04 0.72 ± 0.11 2.5 ± 1 0.7 ± 0.4 54
Debris disks
97 HD 225200 < 1.7 ± 0.5 – <3.03 – 2
98 †HD 2772 <0.84 – < 1.4 ± 1.8 – 2
99 HD 14055 <0.47 4.3 ± 2.4 < 0.8 ± 1.7 6.4 ± 1.1 2, 47
100 HD 15115 <2.48 2.6 ± 0.6 < 4.4 ± 1.9 8.5 ± 1.2 2, 48, 47
101 HD 17848 < 5.4 ± 0.5 – <10.06 – 2
102 †HD 21620 <0.91 – < 1.5 ± 1.8 – 2
103 †HD 23642 0.710 ± 0.18 – < 1.4 ± 1.8 – 2
104 HD 24966 < 1.6 ± 0.5 – <2.75 – 2
105 HD 30422 < 1.2 ± 0.5 – <2.13 – 2
106 HD 31295 <1.1 – < 1.9 ± 1.8 – 2
107 HD 35850 < 1.3 ± 0.5 – <2.17 <5.4 2
108 HD 38206 < 1.5 ± 0.5 – <2.67 – 2
109 β Pic 3.6 ± 3.9 34 ± 18 6.59 ± 0.69 60 ± 6 49
110 HD 42111 <1.21 – < 2.1 ± 1.8 – 2
111 HD 54341 < 1.4 ± 0.5 – <2.39 – 2
112 HD 71043 < 1.5 ± 0.5 – <2.64 – 2
113 HD 71155 < 1.5 ± 0.5 – <2.56 – 2
114 HD 78702 < 1.2 ± 0.5 0.3 ± 1.9 <2.03 0.3 ± 2.3 2
115 HD 136246 < 1.4 ± 0.5 – <2.37 – 2
116 †HD 159082 <0.66 – < 1.1 ± 1.8 – 2
117 HD 164249 < 1.3 ± 0.5 – <2.29 – 2
118 HD 166191 < 1.5 ± 0.5 – <2.66 – 2
119 HD 181296 < 1.2 ± 0.5 9.1 ± 3.7 <2.11 14.4 2
120 HD 182681 < 1.6 ± 0.5 3.4 ± 2.1 <2.79 5 ± 1.3 2, 47
121 HD 218396 <0.5 20 < 0.8 ± 1.7 10.3 ± 1.8 2, 50
122 HD 220825 < 1.3 ± 0.5 – <2.2 – 2

Notes. Objects are sorted first by category and then by increasing RA values are presented here as given in the literature. For some rare cases, there are no errorbars. Values in italics correspond to extrapolation from the other frequency. Values given with the symbol “<” followed by an errorbar (e.g. <1.5 ± 0.5) correspond to sources observed with ALMA where confusion with surrounding molecular clouds partly affects the emission from the source. Upper limits are 3σ.

(1)

The flux of AB Aur is contaminated by the envelope. We have estimated the emission of the disk to be ≈80 Jy km s-1 from interferometric observations with PdBI.

(†)

Binary stars.

Reference. 1 – Ricci et al. (2014); 2 – this work; 3 – Williams & Best (2014); 4 – Guilloteau et al. (2011); 5 – Andrews & Williams (2005); 6 – Koerner & Sargent (1995); 7 – Beckwith et al. (1990); 8 – Thi et al. (2001); 9 – Akeson & Jensen (2014); 10 – Mannings & Emerson (1994); 11 – Öberg et al. (2010); 12 – Andrews & Williams (2007); 13 – Duvert et al. (2000); 14 – Ansdell et al. (2015); 15 – Rodriguez et al. (2015); 16 – Dent et al. (2005); 17 – Brown et al. (2009); 18 – Perez et al. (2015); 19 – Zuckerman et al. (1995); 20 – Natta et al. (2004b); 21 −Zhang et al. (2014); 22 – Tsukagoshi et al. (2014); 23 – Romero et al. (2012); 24 – Salyk et al. (2014); 25 – Andrews et al. (2009); 26 −Ricci et al. (2012); 27 −Kastner et al. (2008); 28 – Jensen et al. (1996); 29 – Chapillon et al. (2008); 30 – Isella et al. (2010); 31 −Banzatti et al. (2011); 32 −Panić et al. (2010); 33 – Walsh et al. (2014); 34 – Czekala et al. (2015); 35 – Rosenfeld et al. (2013); 36 – Isella et al. (2007); 37 −Raman et al. (2006); 38 – Hardy et al. (2015); 39 – Hughes et al. (2008); 40 – Sheret et al. (2004); 41 – Kóspál et al. (2013); 42 – Moór et al. (2013); 43 – Moór et al. (2015); 44 – Nilsson et al. (2010); 45 – Pericaud et al. (in prep.); 46 – Sylvester et al. (2001); 47 – Panić et al. (2013); 48 −MacGregor et al. (2015); 49 – Dent et al. (2014); 50 – Williams & Andrews (2006); 51 – Caceres et al. (2015); 52 – Williams et al. (2013); 53 – Canovas et al. (2016); 54 – Lieman-Sifry et al. (2016).

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