Table C.3
Cumulative σ3D and cumulative size data (available on Vizier), used to create Figs. 1, 3, and B.1. We give the median and the uncertainties from the upper and lower 95th interquartile range (2σ) at each step. In the online version, the σ3D values are given for all four cumulative trends that are shown in Fig. B.1 and outlined in Appendix B.1.
| Parameter | Unit | Description |
|---|---|---|
| age_step | Myr | The motions/positions of the stellar members of each next youngest cluster were systematically incorporated at each age-step (thus, age ≥ age_step) |
| median_sig3D | km s−1 | Median cumulative σ3D at each age-step |
| e_lo95_sig3D | km s−1 | Lower error determined from the 95th percentile |
| e_up95_sig3D | km s−1 | Upper error determined from the 95th percentile |
| median_size | pc | Median cumulative size at each age-step |
| e_lo95_size | pc | Lower error determined from the 95th percentile |
| e_up95_size | pc | Upper error determined from the 95th percentile |
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