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SPECTRAL PROPERTIES OF COOL STARS: EXTENDED ABUNDANCE ANALYSIS OF 1,617 PLANET-SEARCH STARS

  • Authors: John M. Brewer, Debra A. Fischer, Jeff A. Valenti, and Nikolai Piskunov

2016 The Astrophysical Journal Supplement Series 225 32.

  • Provider: AAS Journals

Caption: Figure 23.

Same as Figure 22 but for the heavier elements. The [Cr/Fe] ratios demonstrate both the high precision we achieve in our abundances and the effects of S/N ratio on their determination. Points in orange (S/N < 100) have more than twice the rms scatter as those in blue (S/N ≥ 100). We have excluded iron from the comparisons since this would result in an uninformative flat line.

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