Comparison of our T_eff (left), log g-values (middle), and microturbulence (right panel) with data from Martins et al. (2015a,b, dots) and Holgado et al. (2018, 2022, circles). A uniform value of ξ =10 km s⁻¹ was adopted for the photospheric layers of the stars in the Martins et al. (2015a,b) work. Different literature results for the same star are connected by black lines. Typical error bars from the Martins et al. (2015a,b) work are indicated in the left and middle panels; the uncertainties from Holgado et al. are slightly smaller, and for the microturbulent velocities they provide only upper limits in many cases.