Fig. 9.
Same as Fig. 8 but for samples observed by Luck & Heiter (2007, LTE, left) and Liu et al. (2014, NLTE, right, with crosses indicating planet host stars). Here we show only their stars with −0.2 ≤ [Fe/H] ≤ +0.2 that have Gaia DR2 parallaxes (290 and 375 stars for Luck & Heiter 2007; Liu et al. 2014, respectively). Evolution tracks are the standard models of Lagarde et al. (2012) computed with [Fe/H] = 0.
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