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Table C.1.

Data relative to the sample of stars defined in Sect. 4.

Column identifier Description Units
APOGEE_ID APOGEE ID in DR14 None
KIC_ID Kepler Input Catalogue ID None
jmag 2MASS J-band magnitude mag
hmag 2MASS H-band magnitude mag
kmag 2MASS KS-band magnitude mag
ra Right Ascension deg
dec Declination deg
FE_H_APOGEE APOGEE [Fe/H] (DR14) None
ALPHA_M_APOGEE APOGEE [α/M] (DR14) None
age Age from PARAM (R1) Gyr
mass Mass from PARAM (R1) M
rad Radius from PARAM (R1) R
dist Distance from PARAM (R1) kpc
Av Extinction from PARAM (R1) None
evstate Evolutionary state from Yu et al. (2018). RGB = 1, core-He-burning = 2 None
zmax Maximum vertical excursion in MWPotential2014 kpc
ecc Orbit eccentricity in MWPotential2014 None
rperi Pericentre radius in MWPotential2014 kpc
rap Apocentre radius in MWPotential2014 kpc
GALR Position (Galactocentric cylindrical coordinates): Galactocentric radius kpc
GALPHI Position: azimuth rad
GALZ Position: height above the Galactic midplane kpc
vR Galactocentric radial velocity km s−1
vT Galactocentric tangential velocity km s−1
vz Galactocentric vertical velocity km s−1

Notes. Photometric and spectroscopic constraints are taken from 2MASS (Skrutskie et al. 2006) and APOGEE DR14 (Abolfathi et al. 2018). Orbital parameters are computed as described in Sect. 2.2. Ages, masses, radii, distances and extinction are inferred using PARAM’s modelling run R1 (see Table 1). All relevant columns are accompanied by an associated uncertainty, defined either as the standard deviation or the 16th and 84th percentiles. Uncertainties are found in accompanying columns labelled with the suffix “err”.

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