The Fe I 4377 Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis
Katlyn L. Hobbs, Christopher A. Watson, Jean C. Costes, Yvonne Unruh, Dana Clarice Yaptangco, Krishnamurthy Sowmya, Mitchell E. Young, Ernst J. W. de Mooij, Alexander G. M. Pietrow, Pál Váradi Nagy, Alexander I. Shapiro, Veronika Witzke, Federica Rescigno, Ryan A. Rubenzahl, Megan Bedell, Andrew Collier Cameron, Xavier Dumusque, Sean M. O'Brien, Benjamin M. J. Cadell, Baptiste Klein, Niamh Mallaghan, Niamh K. O'Sullivan, Toby Rodel, Sara Tavella
Queen's University Belfast · Queen's University Belfast · Queen's University Belfast · Imperial College London · Imperial College London · University of Graz · Queen's University Belfast · Queen's University Belfast · Leibniz-Institut für Astrophysik Potsdam · Independent Researcher · Max-Planck-Institut für Sonnensystemforschung · University of Graz · University of Birmingham · Flatiron Institute · Flatiron Institute · University of St Andrews · University of Geneva · Queen's University Belfast · Queen's University Belfast · University of Oxford · Queen's University Belfast · University of Oxford · Queen's University Belfast · University of Geneva
astro-ph.SR, astro-ph.EP, astro-ph.IM
Submitted: 2026-07-31
Comments: 16 pages, 12 figures. Accepted for publication in MNRAS
Code: https://github.com/melix/astro4j
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Disentangling stellar activity and planetary signals
- Precise Radial Velocities
- Extreme Precision Radial Velocity Working Group Final Report
- Data-Driven Modeling of Telluric Features and Stellar Variability with StellarSpectraObservationFitting.jl
- EXPRES: A Next Generation RV Spectrograph in the Search for Earth-like Worlds
- HARPS3 for a Roboticized Isaac Newton Telescope
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