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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 5.

Ranges of each of our seven line lists over the full NEID wavelength range (3800–9300 Å). The wavelengths of the lines in each line list are generally uniformly distributed blueward of ∼6500 Å, with a notable gap between 6500-9000 Å populated by only a couple of lines.

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