Comparing T_eff (top) and log g (bottom) derived from the SAPP with corresponding parameters based on interferometric angular diameters (Boyajian et al. 2012; Rabus et al. 2019). The black dashed line in both panels corresponds to the 1:1 ratio and the grey dotted line in the top panel corresponds to a linear fit to the values from Boyajian et al. (2012). We excluded the outlier GJ 725B for which the SAPP derived a T_eff of roughly 3550 K (leftmost blue square in top panel) from the linear fit, for reasons discussed in the text. We note that the K3 dwarf GJ 105A with T_eff ∼4600 K is not shown in the figures.