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Table 3
Kinematic parallax of the Pleiades derived from different subgroups in our sample of cluster members selected by the CPSM.
| Sample | Stars | Mean ± SEM | Median | SD |
| (mas) | (mas) | (mas) | ||
|
|
||||
| p ≥ 0.7500 | 1209 | 7.44 ± 0.01 | 7.46 | 0.42 |
| p ≥ 0.9545 | 1146 | 7.44 ± 0.01 | 7.46 | 0.41 |
| p ≥ 0.9975 | 789 | 7.47 ± 0.01 | 7.47 | 0.34 |
|
|
||||
| radius ≤ 2° | 809 | 7.46 ± 0.01 | 7.46 | 0.37 |
| radius ≤ 3° | 1024 | 7.46 ± 0.01 | 7.46 | 0.39 |
| radius ≤ 5° | 1189 | 7.45 ± 0.01 | 7.46 | 0.41 |
Notes. We provide for each sample the number of stars, mean, standard error of the mean (SEM), median and standard deviation (SD) values.
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