Table 2
Summary of the reference data: parameter ranges, uncertainties, and provenance.
| Sample | Dist. range [kpc] | σ(Teff) [K] | Teff range [K] | σlog g | log g range | σ [Fe/H] | [Fe/H] range | photom. | Magnitude range |
|
|
|||||||||
| Simulated sample | 0.1−6 | 100 | 3000−7000 | 0.1 | 1.0−5.0 | 0.1 | − 2.2−0.5 | JH Ks | distance-limited |
| Hipparcos-Bensby | < 0.3 1 | 30−100 2 | 4800−7000 | 0.1 | 3.0−4.8 | 0.1 | − 2.5−0.5 | B T V T 3 | V< 9 2 |
| Hipparcos-APOGEE | < 0.3 1 | 90 | 3800−5500 | 0.2 | 1.0−4.0 | 0.1 | ~ − 1.0−0.5 | JH K s 5 | (J−K)0> 0.5;H< 7 |
| CoRoT-APOGEE | 1−6 4 | 100 4 | 4000−5300 | 0.05 | 1.6−3.0 | 0.1 | − 0.8−0.5 | JH K s 5 | (J−K)0> 0.5;H< 13.8 4 |
| APOGEE Clusters | 1−12 6,7 | 100 8 | 3700−5000 | 0.2 | 1.0−3.4 | 0.1 | − 1.0−0.5 | JH K s | (J−K)0> 0.5;H< 13.8 9 |
| SEGUE Clusters | 1−12 6,7 | 130 10 | 4700−7000 | 0.21 | 1.6−5.0 | 0.11 | − 3.0−0.0 | ugriz 11 | 0.48 < (g−r)0< 0.55;r0< 20.2 12 |
Notes. log g values in the CoRoT-APOGEE sample are based on asteroseismic measurements. All other non-photometric parameters were derived spectroscopically; the relevant references are given in the footnotes indicated in the third column.
Reference. (1) van Leeuwen (2007); (2) Bensby et al. (2014); (3) Høg et al. (2000); (4) Anders et al. (2015) and references therein; (5) Cutri et al. (2003); (6) WEBDA Database; (7) Harris (1996); (8) Ahn et al. (2014); (9) Zasowski et al. (2013); (10) Ahn et al. (2012); (11) Fukugita et al. (1996); (12) Lee et al. (2008a).
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