Parameter estimates from the KIC plotted against estimates by D. Fischer from SME model spectrum fitting, for stars observed with the Keck/HIRES spectrometer as possible transiting planet hosts. A few stars have more than one independent HIRES/SME observation and analysis; in these cases, the various results are shown connected by horizontal lines. Panel (a) shows T _eff on each axis, with lines showing equality and ±200 K overplotted. Panel (b) shows log ( g), with lines showing equality and ±0.3 dex. Panel (c) similarly shows log ( Z), with line showing equality and ±0.4 dex.