Fig. 6
Top panel: [C/Fe] distributions of three different samples: stars without planets (NP, in red), low-mass planets (LMP, in green), and high-mass planets (HMP, in blue). Middle panel: [C/H] distributions for the three mentioned samples. Bottom panel: [C/H] distributions for the same three groups, but considering only solar analogues (Teff = Teff, ⊙ ± 300 K).
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