Fig. 15
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[C/Fe], [N/Fe], [O/Fe], and [S/Fe] vs. Mp. Asterisks represent binned values for Mp (< 0.4, 0.4–0.6, 0.6–1.2, 1.2–2.4, > 2.4 MJup) and the error bars show the standard deviation for each bin. The targets with Mp < 0.4 MJup and Mp > 2.4 MJup are labeled. The gray points for carbon and nitrogen are the values obtained for planet-hosting stars by Suárez-Andrés et al. (2016, 2017), respectively. The dashed lines represent the solar values.
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