The MUSCLES Treasury Survey. IV. Scaling Relations for Ultraviolet, Ca ii K, and Energetic Particle Fluxes from M Dwarfs

The MUSCLES Treasury Survey. IV. Scaling Relations for Ultraviolet, Ca ii K, and Energetic Particle Fluxes from M Dwarfs

Characterizing the UV spectral energy distribution (SED) of an exoplanet host star is critically important for assessing its planet's potential habitability, particularly for M dwarfs, as they are prime targets for current and near-term exoplanet characterization efforts and atmospheric models...

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Main Authors: Youngblood, Allison (Author), France, Kevin (Author), Loyd, R. O. Parke (Author), Brown, Alexander (Author), Mason, James P. (Author), Schneider, P. Christian (Author), Tilley, Matt A. (Author), Berta-Thompson, Zachory K. (Author), Buccino, Andrea (Author), Froning, Cynthia S. (Author), Hawley, Suzanne L. (Author), Linsky, Jeffrey (Author), Mauas, Pablo J. D. (Author), Redfield, Seth (Author), Kowalski, Adam (Author), Miguel, Yamila (Author), Rugheimer, Sarah (Author), Segura, Antígona (Author), Roberge, Aki (Author), Vieytes, Mariela (Author), Newton, Elisabeth R (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-11-08T18:57:02Z.
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