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Revisiting ϵ Eridani with NEID: Identifying New Activity-sensitive Lines in a Young K Dwarf Star

  • Authors: Sarah Jiang, Arpita Roy, Samuel Halverson, Chad F. Bender, Carlos Selgas, O. Justin Otor, Suvrath Mahadevan, Guđmundur Stefánsson, Ryan C. Terrien, Christian Schwab

Sarah Jiang et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 2.

Examples of the visual criteria we used to prune our line lists. We determine whether or not to remove a line based on whether the Gaussian fit appears to accurately fit and measure a line’s parameters, and if the correlations appear to exhibit a significant outlier that skews the correlation. (a) An example of a “good” line that we do not remove, since the Gaussian fit appears to match the line within its wings. (b) An example of a noisy line such that the Gaussian fit does not accurately fit the line. (c) An example of a blended line with multiple peaks in the fitting window, such that the Gaussian fit does not accurately fit the line. (d) An example of a line whose plot correlating line depth with the S-index exhibits a significant outlier that skews the best-fit line.

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