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 nearterm exoplanet characterization efforts and atmospheric models predic...

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Bibliografiska uppgifter
Huvudupphovsmän:	Youngblood, A, France, K, Loyd, R, Brown, A, Mason, J, Schneider, P, Tilley, M, Berta-Thompson, Z, Buccino, A, Froning, C, Hawley, S, Linsky, J, Mauas, P, Redfield, S, Kowalski, A, Miguel, Y, Newton, E, Rugheimer, S, Segura, A, Roberge, A, Vieytes, M
Materialtyp:	Journal article
Publicerad:	Institute of Physics 2017

The MUSCLES Treasury Survey. IV. Scaling relations for ultraviolet, Ca ii K, and energetic particle fluxes from M dwarfs

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