Table C.1
Cluster statistics for the different disk selection samples that are used to determine five different disk fractions.
| Cluster name | Age (Myr) | CCD | SED | Luhman a | RUWE < 1.4 | RUWE ≥ 1.4 | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| DB | DL | fdisks | DB | DL | fdisks | DB | DL | fdisks | DB | DL | fdisks | DB | DL | fdisks | ||
| rho Oph/L1688 | ![]() |
164 | 278 | ![]() |
183 | 259 | ![]() |
140 | 230 | ![]() |
141 | 243 | ![]() |
23 | 35 | ![]() |
| nu Sco | ![]() |
39 | 89 | ![]() |
40 | 88 | ![]() |
39 | 84 | ![]() |
33 | 72 | ![]() |
6 | 17 | ![]() |
| delta Sco | ![]() |
111 | 500 | ![]() |
110 | 501 | ![]() |
105 | 479 | ![]() |
95 | 403 | ![]() |
16 | 97 | ![]() |
| beta Sco | ![]() |
51 | 193 | ![]() |
51 | 193 | ![]() |
46 | 167 | ![]() |
40 | 156 | ![]() |
11 | 37 | ![]() |
| sigma Sco | ![]() |
58 | 409 | ![]() |
60 | 407 | ![]() |
40 | 358 | ![]() |
50 | 347 | ![]() |
8 | 62 | ![]() |
| Antares | ![]() |
61 | 367 | ![]() |
57 | 371 | ![]() |
38 | 280 | ![]() |
47 | 296 | ![]() |
14 | 71 | ![]() |
| rho Sco | ![]() |
17 | 185 | ![]() |
21 | 181 | ![]() |
18 | 171 | ![]() |
13 | 154 | ![]() |
4 | 31 | ![]() |
| Scorpio-Body | ![]() |
13 | 217 | ![]() |
12 | 218 | ![]() |
10 | 154 | ![]() |
9 | 172 | ![]() |
4 | 45 | ![]() |
| US-foreground | ![]() |
4 | 217 | ![]() |
7 | 214 | ![]() |
2 | 83 | ![]() |
3 | 186 | ![]() |
1 | 31 | ![]() |
| V1062-Sco | ![]() |
55 | 518 | ![]() |
46 | 528 | ![]() |
22 | 451 | ![]() |
43 | 425 | ![]() |
12 | 93 | ![]() |
| mu Sco | ![]() |
4 | 24 | ![]() |
2 | 26 | ![]() |
2 | 24 | ![]() |
4 | 19 | ![]() |
0 | 5 | ![]() |
| Libra-South | ![]() |
0 | 59 | ![]() |
0 | 59 | ![]() |
1 | 53 | ![]() |
0 | 51 | ![]() |
0 | 8 | ![]() |
| Lupus-1-4 | ![]() |
84 | 108 | ![]() |
77 | 114 | ![]() |
70 | 81 | ![]() |
59 | 84 | ![]() |
25 | 24 | ![]() |
| eta Lup | ![]() |
27 | 529 | ![]() |
29 | 528 | ![]() |
25 | 444 | ![]() |
24 | 440 | ![]() |
3 | 89 | ![]() |
| phi Lup | ![]() |
55 | 865 | ![]() |
57 | 864 | ![]() |
54 | 748 | ![]() |
46 | 704 | ![]() |
9 | 161 | ![]() |
| e Lup | ![]() |
15 | 394 | ![]() |
16 | 394 | ![]() |
14 | 354 | ![]() |
15 | 332 | ![]() |
0 | 62 | ![]() |
| UPK606 | ![]() |
8 | 98 | ![]() |
9 | 98 | ![]() |
9 | 87 | ![]() |
6 | 84 | ![]() |
2 | 14 | ![]() |
| rho Lup | ![]() |
17 | 179 | ![]() |
18 | 178 | ![]() |
13 | 169 | ![]() |
14 | 149 | ![]() |
3 | 30 | ![]() |
| nu Cen | ![]() |
117 | 1385 | ![]() |
131 | 1373 | ![]() |
116 | 1219 | ![]() |
103 | 1185 | ![]() |
14 | 200 | ![]() |
| sig Cen | ![]() |
129 | 1244 | ![]() |
125 | 1250 | ![]() |
94 | 995 | ![]() |
108 | 1025 | ![]() |
21 | 219 | ![]() |
| Acrux | ![]() |
26 | 222 | ![]() |
19 | 229 | ![]() |
14 | 199 | ![]() |
22 | 161 | ![]() |
4 | 61 | ![]() |
| Musca-foreground | ![]() |
15 | 72 | ![]() |
15 | 72 | ![]() |
10 | 40 | ![]() |
12 | 57 | ![]() |
3 | 15 | ![]() |
| eps Cham | ![]() |
8 | 22 | ![]() |
7 | 23 | ![]() |
… | … | ⋯ | 7 | 15 | ![]() |
1 | 7 | ![]() |
| eta Cham | ![]() |
8 | 21 | ![]() |
7 | 21 | ![]() |
⋯ | ⋯ | ⋯ | 7 | 15 | ![]() |
1 | 6 | ![]() |
| B59 | ![]() |
15 | 5 | ![]() |
15 | 5 | ![]() |
… | ⋯ | … | 9 | 4 | ![]() |
6 | 1 | ![]() |
| Pipe-North | ![]() |
4 | 30 | ![]() |
4 | 30 | ![]() |
… | ⋯ | ⋯ | 2 | 25 | ![]() |
2 | 5 | ![]() |
| tet Oph | ![]() |
1 | 51 | ![]() |
0 | 53 | ![]() |
2 | 42 | ![]() |
1 | 41 | ![]() |
0 | 10 | ![]() |
| CrA-Main | ![]() |
23 | 57 | ![]() |
21 | 59 | ![]() |
… | ⋯ | ⋯ | 18 | 49 | ![]() |
5 | 8 | ![]() |
| CrA-North | ![]() |
33 | 246 | ![]() |
34 | 247 | ![]() |
4 | 44 | ![]() |
29 | 206 | ![]() |
4 | 40 | ![]() |
| Scorpio-Sting | ![]() |
3 | 63 | ![]() |
2 | 64 | ![]() |
2 | 50 | ![]() |
2 | 51 | ![]() |
1 | 12 | ![]() |
| Chamaeleon-1 | ![]() |
68 | 75 | ![]() |
66 | 72 | ![]() |
⋯ | ⋯ | ⋯ | 51 | 65 | ![]() |
17 | 10 | ![]() |
| Chamæleon-2 | ![]() |
30 | 10 | ![]() |
30 | 10 | ![]() |
⋯ | ⋯ | ⋯ | 23 | 6 | ![]() |
7 | 4 | ![]() |
| L134/L183 | ![]() |
3 | 18 | ![]() |
3 | 18 | ![]() |
⋯'. | ⋯ | ⋯ | 2 | 9 | ![]() |
1 | 9 | ![]() |
Notes. Col. 1 gives the cluster name, and Col. 2 gives the cluster age and their uncertainties from Ratzenböck et al. (2023b). Cols. 3–17 give the resulting disk statistics per disk selection, showing disk-bearing (DB), disk-less (DL), and the disk fraction (including 1σ lower and upper confidence interval) for each of the five cases. The first three groups are the CCD, SED, and Luhman selections. The RUWE subsamples are based on the CCD selection, to separate the sample into possible single-star candidates (RUWE < 1.4) and binary candidates (RUWE ≥ 1.4). aDisk selection from Luhman (2022).
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