Table A.1
Targets excluded from our analysis.
| 2MASS ID | Reason |
|---|---|
| 11143442-4418240 | ϖ = (1.94 ± 0.01) mas < 4 mas |
| 11472064-4953042 | No astrometric measurements |
| 12063292-4247508 | μ = (56.5 ± 0.1) mas yr−1 > 55 mas yr−1 |
| 12124890-6230317 | No astrometric measurements |
| 12253370-7227480 | No astrometric measurements |
| 13010856-5901533 | No astrometric measurements |
| 13032904-4723160 | No astrometric measurements |
| 13405585-4244505 | No astrometric measurements |
| 15151856-4146354 | σϖ = 0.55 mas > 0.50 mas |
| 15250358-3604455 | σϖ = 0.57 mas > 0.50 mas |
| 15272286-3604087 | No astrometric measurements |
| 15280322-2600034 | ϖ = (1.76 ± 0.06) mas < 4 mas |
| 15364094-2923574a | Optical triple |
| 15374917-1840449 | ϖ = (0.76 ± 0.03) mas < 4 mas |
| 15455225-4222163 | No astrometric measurements |
| 15463111-5216580 | No astrometric measurements |
| 15494499-3925089 | No astrometric measurements |
| 15550624-2521102 | No astrometric measurements |
| 15564402-4242301 | No astrometric measurements |
| 16003134-2027050 | No astrometric measurements |
| 16015149-2445249 | No astrometric measurements |
| 16021045-2241280 | No astrometric measurements |
| 16025243-2402226 | ϖ = (0.82 ± 0.02) mas < 4 mas |
| 16025396-2022480 | No astrometric measurements |
| 16034536-4355492 | No astrometric measurements |
| 16062196-1928445 | No astrometric measurements |
| 16070356-2036264 | No astrometric measurements |
| 16120140-3840276 | No astrometric measurements |
| 16131738-2922198 | No astrometric measurements |
| 16141107-2305362 | ϖ = (0.50 ± 0.11) mas < 4 mas |
| 16195068-2154355 | No astrometric measurements |
| 16240632-2456468 | No astrometric measurements |
| 16271951-2441403 | No astrometric measurements |
| 16384946-2735294 | ϖ = (3.73 ± 0.72) mas < 4 mas |
Notes. The targets in the table were excluded from the analysis, either because they were not consistent with Sco-Cen membership according to the criteria listed in de Zeeuw et al. (1999) and Pecaut & Mamajek (2016) or the Gaia database contained insufficient or uncertain astrometric information.(a) 2MASS J15364094-2923574 is resolved by Gaia into an optical triple, comprised of a foreground (ϖ ≃ 16 mas), high proper motion, physical binary (Gaia EDR3 6209195913018942976 & Gaia EDR3 6209195913018942720) and a third background interloper (Gaia EDR3 6209195913015396608).
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