Table A.6.
Gaia parallaxes, proper motions and calculated reduced proper motions, distances, absolute G magnitudes and reddening of central stars of planetary nebula from Miszalski et al. (2009).
| Target | Parallax | Proper motion in RA | Proper motion in Dec | MG | Reduced proper motion | Distance | Distance (Bailer-Jones et al. 2018) | AG | E(B − V) | Reddening corrected MG |
|---|---|---|---|---|---|---|---|---|---|---|
| mas | mas yr−1 | mas yr−1 | mag | kpc | kpc | |||||
| OGLE-BLG-ECL-000111 (1) | −0.6078 ± 0.3030 | −1.016 ± 0.451 | −4.317 ± 0.403 | − | 11.59 ± 0.43 | – |
 |
1.48 | 0.5 |
 |
| OGLE-BLG-ECL-159262 (3) | 0.8984 ± 0.5485 | −6.094 ± 0.961 | −8.566 ± 0.739 | 8.85 ± 1.32 | 14.20 ± 0.19 | 1.113 ± 0.679 |
 |
1.49 | 0.5 |
 |
| J277.8274+26.9367 (4) | 0.3286 ± 0.0440 | −1.936 ± 0.052 | 0.692 ± 0.070 | 2.52 ± 0.29 | 6.5 ± 0.39 | 3.099 ± 0.415 |
 |
Notes. (1)Discovered by Soszyński et al. (2015). (2)Discovered by visual inspection. (3)Discovered by machine-learning. (4)Discovered by Pietrukowicz et al. (2013). (5)Discovered by cross-match of the sdB candidate catalogue (Geier et al. 2019) with the ATLAS survey.
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