Image Details
Caption: Figure 3.
[Fe/H] and [α/Fe] of TOI-7019 in comparison to the allStarLite-dr17 APOGEE sample. We have shifted the APOGEE sample by +0.04 in [α/Fe] to account for a systematic offset between the [α/Fe] from APOGEE and that measured by UberMS (E. K. Pass et al. 2025). The dashed blue line indicates a typical selection that separates the high-α (thick) and low-α (thin) disk.
© 2026. The Author(s). Published by the American Astronomical Society.