Image Details
Caption: Figure 6.
Comparison of the metallicity calibration sample from A. W. Mann et al. (2013; black points) to our measured metallicity of TOI-5205 (red point). The metallicities are shown plotted against host-star spectral type. Our measured metallicity is at the upper limit of the calibration sample.
© 2026. The Author(s). Published by the American Astronomical Society.