Same as the previous figure, except for stars with T _eff and log ( g) estimates from matching a grid of models to reconnaissance spectroscopy of Kepler transiting planet candidates. Most plotted points are the average of results from two or more independent spectra. Also, small random offsets have been applied in both axes, to reduce crowding. Diagonal lines indicate equality and ±250 K, ±0.3 dex. The analysis of these spectra provided no metallicity estimates, so log ( Z) is not shown.