Table A.2.
Median proper motions and their uncertainties for the colour bins in the CMD Ks versus H − Ks.
| H − Ks | #stars | μl | dμl | σμl | μb | dμb | σμb |
|---|---|---|---|---|---|---|---|
| (mag) | (mas/yr) | (mas/yr) | (mas/yr) | (mas/yr) | (mas/yr) | (mas/yr) | |
| 1.3-1.5 | 131 | 2.37 | 0.30 | 2.79 | 0.04 | 0.23 | 2.15 |
| 1.5-1.7 | 267 | 1.69 | 0.22 | 2.82 | 0.07 | 0.18 | 2.37 |
| 1.7-1.9 | 439 | 0.53 | 0.16 | 2.67 | 0.04 | 0.14 | 2.42 |
| 1.9-2.1 | 489 | 0.08 | 0.17 | 2.94 | -0.08 | 0.15 | 2.57 |
| 2.1-2.3 | 364 | 0.01 | 0.19 | 2.88 | -0.28 | 0.16 | 2.46 |
| 2.3-2.5 | 247 | -0.12 | 0.21 | 2.63 | 0.08 | 0.20 | 2.46 |
| 2.5-2.7 | 135 | -0.03 | 0.28 | 2.64 | -0.26 | 0.29 | 2.66 |
| 2.7-2.9 | 63 | -0.51 | 0.46 | 2.90 | -0.18 | 0.38 | 2.40 |
Notes. H − Ks, μi, dμi, and σμi indicate the approximate colour range (see Fig. 3) and the median value of the proper motion distribution with its corresponding standard error and the standard deviation, respectively. The subindex i indicates Galactic longitude (i = l) or latitude (i = b).
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