Reconstructing the extreme ultraviolet emission of cool dwarfs using differential emission measure polynomials

Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZMAT, and FUMES have collected multiwavelength spectra across the spectral type's range of Teff and activity, but th...

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Bibliographic Details
Main Authors:	Duvvuri, GM, Sebastian Pineda, J, Berta-Thompson, ZK, Brown, A, France, K, Kowalski, AF, Redfield, S, Tilipman, D, Vieytes, MC, Wilson, DJ, Youngblood, A, Froning, CS, Linsky, J, Parke Loyd, RO, Mauas, P, Miguel, Y, Newton, ER, Rugheimer, S, Schneider, PC
Format:	Journal article
Language:	English
Published:	IOP Publishing 2021

Reconstructing the extreme ultraviolet emission of cool dwarfs using differential emission measure polynomials

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