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...
Main Authors: | , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | |
Format: | Article |
Published: |
IOP Publishing
2017
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Online Access: | http://hdl.handle.net/1721.1/112150 |