Image Details
Caption: Figure 10.
The difference between MWM [M/H] and literature [Fe/H] as a function of ASPCAP raw Teff and log g from APOGEE DR17 (top panels), GALAH DR4 (second row from the top), Gaia-ESO DR5 (second row from the bottom) for stars with S/N > 50 from both surveys, and no BAD flags from MWM. The bottom panels show the comparison with the GBS sample. The solid black line shows the running median value.
© 2025. The Author(s). Published by the American Astronomical Society.