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Table 2.

Proper motions and parallaxes of the Lupus subgroups in our sample of cluster members.

Sample Ninit NRUWE μα cos δ μδ ϖ
(mas yr−1)
(mas yr−1)
(mas)
Mean ± SEM Median SD Mean ± SEM Median SD Mean ± SEM Median SD
Lupus 1 6 4 −12.414 ± 0.387 −12.446 0.773 −23.002 ± 0.439 −22.848 0.878 6.442 ± 0.069 6.447 0.139
Lupus 2 5 2 −11.875 ± 0.216 −11.875 0.433 −23.335 ± 0.383 −23.335 0.767 6.283 ± 0.028 6.283 0.056
Lupus 3 61 56 −10.118 ± 0.113 −9.986 0.843 −23.541 ± 0.095 −23.492 0.710 6.262 ± 0.020 6.272 0.148
Lupus 4 22 18 −10.997 ± 0.177 −11.006 0.753 −23.361 ± 0.125 −23.348 0.532 6.190 ± 0.027 6.194 0.116
Lupus 5 3 2 −8.684 ± 0.121 −8.684 0.241 −24.313 ± 0.217 −24.313 0.434 6.477 ± 0.091 6.477 0.182
Lupus 6 1 1 −9.669 ± 0.125 −9.669 −23.718 ± 0.094 −23.718 6.663 ± 0.053 6.663
Lupus (off-cloud) 39 30 −10.259 ± 0.263 −10.254 1.443 −23.162 ± 0.143 −22.954 0.782 6.256 ± 0.042 6.273 0.231

Lupus (all stars) 137 113 −10.378 ± 0.109 -10.306 1.155 −23.404 ± 0.068 −23.387 0.721 6.263 ± 0.017 6.265 0.178

Notes. We provide for each subgroup the initial number of stars, final number of stars after the RUWE filtering (see Sect. 4.1), mean, standard error of the mean (SEM), median, and standard deviation (SD) of proper motions and parallaxes.

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