Mean T_cond slope (﹩\frac{\partial [{\rm{X}}/{\rm{Fe}}]}{\partial {T}_{{\rm{cond}}}}﹩) as a function of mean T_eff and colored by mean ﹩\mathrm{log}g﹩ for stars with the same [Fe/H] and [α/Fe] consistent with the Sun with B18 as circles (only one symbol shown since these stars occupy one bin), GALAH as squares, R24 as diamonds, and APOGEE as stars. There is a slight negative gradient in T_cond slope with T_eff for each dataset (-3 ± 1E-7 dex/K²) and with ﹩\mathrm{log}g﹩ (-1 ± 3E-4 K²). Hotter and lower ﹩\mathrm{log}g﹩ stars tend to share ﹩\frac{\partial [{\rm{X}}/{\rm{Fe}}]}{\partial {T}_{{\rm{cond}}}}﹩ = 0 than stars with similar T_eff and ﹩\mathrm{log}g﹩ as the Sun. The APOGEE stars are systemically offset from the rest of the surveys, given their difference in kinematic selection as shown in Figure 4.