Fig. 6
Comparison between our abundances and previous results in the literature (R03: Reddy et al. 2003; VF05: Valenti & Fischer 2005; M08: Mishenina et al. 2008; GM06: Gillon & Magain 2006; B04: Bruntt et al. 2004). The results for HD 42618 and HD 43587 are shown with circles and triangles, respectively. Our abundances based on a single spectral line have their uncertainty conservatively set to 0.05 dex.
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