Parameters from the LPV pipeline for the bright late-type stars of Messineo & Brown (2019). Left panel: Per values versus Ampl values of the Gaia variables. The dotted line is drawn by eye to separate the outliers (dark green) from the bulk of the distribution (red). Right panel: bolometric magnitudes versus T_eff values of late-type stars from Messineo & Brown (2019) are marked with gray circles. Red and dark green symbols are those with measured Gaia Per values, as in the left panel.