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Table 3
Summary of the results for the reference distance samples we used.
| Sample | Nstars | Dist. range [kpc] | Mean rel. residuals [%] | rms rel. residuals [%] |
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| Simulated “high-res.” stars | 5000 | 0.1−6 | + 1.2 | 20.9 |
| Dwarfs (log g> 4) | 1248 | 0.1−6 | − 0.5 | 10.6 |
| Giants (log g< 4) | 3752 | 0.1−6 | + 1.8 | 23.3 |
| Simulated “low-res.” stars | 5000 | 0.1−6 | + 3.3 | 33.4 |
| Dwarfs (log g> 4) | 1248 | 0.1−6 | − 0.6 | 15.5 |
| Giants (log g< 4) | 3752 | 0.1−6 | + 4.6 | 37.4 |
| Hipparcos-Bensby dwarfs | 714 | ≲ 0.2 | + 0.4 | 18.2 |
| Hipparcos-APOGEE giants | 712 | < 0.3 | + 1.6 | 26.4 |
| CoRoT-APOGEE giants | 644 | 1−12 | + 8.7 | 14.9 |
| APOGEE clusters – cluster age prior | 392 | 1−15 | − 16.5 | 29.9 |
| SEGUE clusters – field priors | 419 | 1−12 | + 14 | 43 |
| Δlog g = + 0.25 dex; field priors | 425 | 1−12 | − 2 | 35 |
| Δlog g = + 0.25 dex; clus. age priors | 385 | 1−12 | + 13 | 39 |
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