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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 4.

Venn diagram of our seven line lists and the number of lines in each list. All numbers/line lists are exclusive; i.e., we found nine lines correlated with the S-index in all three parameters (depth, FWHM, and integrated flux), 55 lines correlated with the S-index in depth and FWHM only, 79 lines correlated with the S-index in depth and integrated flux only, six lines correlated with the S-index in FWHM and integrated flux only, and 167, 131, 44 lines respectively correlated with the S-index in depth, FWHM, or integrated flux only.

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