Table 1.
Summary of the completeness of the sample for four different distance ranges.
| Total # | % obs. | Total # | % obs. | |
|---|---|---|---|---|
| Bmag ≤ 9 | Bmag ≤ 9 | 9 < Bmag ≤ 11 | 9 < Bmag ≤ 11 | |
| Distance 0–1000 pc | ||||
| Any δ | 83 | 80% | 2 | 50% |
| δ > −20 | 59 | 80% | 1 | 0% |
| Distance 1000–2000 pc | ||||
| Any δ | 265 | 77% | 173 | 27% |
| δ > −20 | 150 | 90% | 104 | 38% |
| Distance 2000–3000 pc | ||||
| Any δ | 235 | 61% | 431 | 21% |
| δ > −20 | 105 | 91% | 234 | 34% |
| Distance 3000–4000 pc | ||||
| Any δ | 68 | 47% | 205 | 13% |
| δ > −20 | 26 | 73% | 123 | 15% |
Notes. For each distance range, we include the statistics for stars in the green and blue regions, where stars of each kind are described as in Sect. 4.2.3 (see also Fig. 11). In particular, the first two columns indicate the total number of stars with Bmag < 9, and the corresponding percentage of observed stars with respect to the total. The last two columns indicate the same, but for stars with 9 < Bmag < 11.
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