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Table 1

Bayesian expansion ages of local young stellar associations.

RV Members Distance Age

Origin Coverage final μ ± σ
% (pc) (Myr)
Association Membership
EPCHA SigMA GLASSS 37.8 37 102 6.4 ± 2.1
MuscaFG UNION-A GLASSS 53.8 39 101 10.4 ± 1.4
ETCHA UNION GLASSS 60.0 20 98 7.6 ± 3.4
TWA L23-A GLASSS 58.5 41 63 10.2 ± 1.0
L23-B GLASSS 53.3 15 65 8.5 ± 1.3
118TAU UNIONS+L22-A GLASSS 60.0 35 107 24.0 ± 4.5
THOR UNIONS+L22-B GLASSS 66.7 45 101 29.8 ± 4.9
Háap UNIONS+L22-C GLASSS 55.6 63 90 25.9 ± 4.6
BPIC Miret-Roig+2020 Original 73.1 26 42 23.4 ± 4.8
Balaam Luhman2024-B Original 47.6 63 63 19.3 ± 4.7
OCT UNION-A GLASSS 81.2 69 150 30.4 ± 4.6
HSC2597 UNION-C GLASSS 41.2 17 138 39.6 ± 6.9
COL UNION-A GLASSS 59.2 125 71 33.0 ± 9.2
OMAU UNION-C GLASSS 46.7 15 36 40.1 ± 5.9
CAR Luhman2024-AB GLASSS 44.8 259 112 45.4 ± 9.2
Platais8 Luhman2024-AA GLASSS 42.0 362 133 28.3 ± 10.9
Nal Luhman2024-BA GLASSS 11.4 35 183 16.1 ± 5.5
Chem Luhman2024-BB GLASSS 30.3 132 168 22.2 ± 2.1
THA Lee+2019-A GLASSS 58.4 161 42 32.9 ± 6.3
Lee+2019-B GLASSS 54.1 37 43 38.6 ± 5.4

Notes. The columns in this table correspond, from left to right, to the association’s abbreviated name, the selected membership’s list (the reasons for this selection will be described at each LYSA’s section), the RV origin and percentage of coverage (out of the final members), the final number of members (after the decontamination algorithm), the association’s distance, and the inferred Bayesian expansion age. For simplicity, the age is reported as the mean and standard deviation of the inferred age’s posterior distribution. Its 95% HDI (high density interval) is reported in Table B.1.

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