Table B.2
Photometric and astrometric measurements of point sources detected in the first epoch (Cols. 1–5) and the second epoch (Cols. 6–8).
| # | mH2 | mH3 | Separation | PA | mH | Separation | PA | Probability | Status |
|---|---|---|---|---|---|---|---|---|---|
| – | – | – | (mas) | (°) | – | (′′) | (°) | % | – |
| 1 | 16.77 ± 0.08 | 16.78 ± 0.08 | 3338.1 ± 17.0 | 331.33 ± 0.07 | 16.50 ± 0.15 | 3392.5 ± 4.9 | 332.01 ± 0.09 | 13.5 | BS |
| 2 | 20.40 ± 0.08 | 20.28 ± 0.08 | 3451.6 ± 17.6 | 3.43 ± 0.39 | 20.11 ± 0.15 | 3519.7 ± 5.1 | 3.57 ± 0.28 | 71.5 | BS |
| 3 | 22.69 ± 0.19 | 22.56 ± 0.15 | 3694.1 ± 20.5 | 115.71 ± 0.12 | 22.29 ± 0.18 | 3677.7 ± 7.7 | 114.72 ± 0.10 | 93.7 | BS |
| 4 | 19.08 ± 0.08 | 19.02 ± 0.08 | 4091.7 ± 20.8 | 186.52 ± 0.16 | 18.79 ± 0.15 | 4037.2 ± 5.8 | 186.60 ± 0.15 | 57.9 | BS |
| 5 | 22.72 ± 0.16 | 22.57 ± 0.21 | 4143.9 ± 22.7 | 327.61 ± 0.17 | 22.31 ± 0.21 | 4193.3 ± 7.8 | 328.20 ± 0.13 | 97.4 | BS |
| 6 | 17.53 ± 0.08 | 17.58 ± 0.08 | 4154.8 ± 21.1 | 58.29 ± 0.07 | 17.27 ± 0.15 | 4191.2 ± 5.9 | 57.66 ± 0.08 | 30.9 | BS |
| 7 | 21.74 ± 0.10 | 21.74 ± 0.10 | 5046.4 ± 25.8 | 150.21 ± 0.09 | 21.42 ± 0.17 | 4992.9 ± 7.5 | 149.86 ± 0.09 | 98.1 | BS |
| 8 | 19.93 ± 0.08 | 19.93 ± 0.08 | 5376.7 ± 27.3 | 60.42 ± 0.07 | 19.64 ± 0.15 | 5415.8 ± 7.7 | 59.89 ± 0.08 | 90.0 | BS |
| 9 | 21.98 ± 0.13 | 21.93 ± 0.14 | 5616.8 ± 28.9 | 201.19 ± 0.12 | 22.27 ± 0.19 | 5554.2 ± 9.0 | 201.46 ± 0.12 | 99.8 | BS |
| 10 | 21.20 ± 0.19 | 20.71 ± 0.10 | 7009.0 ± 36.0 | 110.91 ± 0.07 | 20.67 ± 0.16 | 6985.8 ± 10.2 | 110.40 ± 0.08 | 99.6 | BS |
| 11 | – | – | – | – | 23.10 ± 0.22 | 6198.7 ± 15.8 | 164.53 ± 0.28 | 100.0 | BS |
| 12 | – | – | – | – | 17.49 ± 0.15 | 7307.9 ± 10.2 | 155.30 ± 0.08 | 72.3 | BS |
| 13 | – | – | – | – | 20.92 ± 0.23 | 7436.4 ± 11.6 | 154.97 ± 0.10 | 100.0 | BS |
| 14 | – | – | – | – | 19.59 ± 0.15 | 7778.4 ± 11.0 | 157.70 ± 0.08 | 98.8 | BS |
| 15 | – | – | – | – | 23.60 ± 0.50 | 2984.7 ± 23.2 | 105.22 ± 0.30 | 89.0 | BS |
Notes. Column 1 is the label in the images shown in Fig. 1, Cols. 2 and 3 are respectively the H2 and H3 relative magnitudes of point sources, Col. 4 is the angular separation to the star of the point sources for the first epoch, Col. 5 is the position angle of the point sources (0° is north andit is counted positive from north to east) for the first epoch, Col. 6 is the BB_H relative magnitude of point sources, Col. 7 is theangular separation to the star of the point sources for the second epoch, Col. 8 is the position angle of the point sources for the second epoch, Col. 9 is the probability of each candidate to be a contaminant background star, based on the Besançon Galaxy Model (Robin et al. 2003), Col. 10 is the current status of candidates (BS: background star).
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