Fig. 13.
Top panel: histogram of temperatures for 239 δ Scuti star candidates observed by CoRoT. Blue bars point to values from COROTSKY database (Charpinet et al. 2006) and red bars point to the values obtained with VOSA (see text). Dotted lines represent the temperature limits for δ Scuti stars (Uytterhoeven et al. 2011). Middle and bottom panels: same as top panel for stars of our main sample observed by Kepler and TESS, respectively.
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