179 citations · 784 across the 23 of their papers we have counts for
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Modeling the Chromosphere and Transition Region of Planet-hosting Star GJ 436
Dominik Hintz, Sarah Peacock, Travis Barman +12
Ahead of upcoming space missions intending to conduct observations of low-mass stars in the ultraviolet (UV) spectral region it becomes imperative to simultaneously conduct atmosph…
HAZMAT. IX. An Analysis of the UV and X-Ray Evolution of Low-Mass Stars in the Era of Gaia
Tyler Richey-Yowell, Evgenya L. Shkolnik, Adam C. Schneider +6
Low mass stars ( M) are some of the best candidates for hosting planets with detectable life because of these stars' long lifetimes and relative planet to star ma…
Accurate Modeling of Lyman-alpha Profiles and their Impact on Photolysis of Terrestrial Planet Atmospheres
Sarah Peacock, Travis S. Barman, Adam C. Schneider +4
Accurately measuring and modeling the Lyman- (Ly; 1215.67 Å) emission line from low mass stars is vital for our ability to build predictive high energy stellar spectra, ye…
HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars
R. O. Parke Loyd, Evgenya L. Shkolnik, Adam C. Schneider +6
The ultraviolet (UV) emission from the most numerous stars in the universe, M dwarfs, impacts the formation, chemistry, atmospheric stability, and surface habitability of their pla…
Estimating the Ultraviolet Emission of M dwarfs with Exoplanets from Ca II and H
Katherine Melbourne, Allison Youngblood, Kevin France +29
M dwarf stars are excellent candidates around which to search for exoplanets, including temperate, Earth-sized planets. To evaluate the photochemistry of the planetary atmosphere,…
HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Star
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik +4
Quantifying the evolution of stellar extreme ultraviolet (EUV, 100 -- 1000 ) emission is critical for assessing the evolution of planetary atmospheres and the h…
Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets Around Low-Mass Stars: GJ 832, GJ 176, GJ 436
Sarah Peacock, Travis Barman, Evgenya Shkolnik +3
Correct estimates of stellar extreme ultraviolet (EUV; 100 - 1170 Å) flux are important for studying the photochemistry and stability of exoplanet atmospheres, as EUV radiation ion…
Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets Around Low-Mass Stars: the TRAPPIST-1 System
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik +2
The high energy radiation environment around M dwarf stars strongly impacts the characteristics of close-in exoplanet atmospheres, but these wavelengths are difficult to observe du…
HAZMAT. IV. Flares and Superflares on Young M Stars in the Far Ultraviolet
R. O. Parke Loyd, Evgenya L. Shkolnik, Adam C. Schneider +4
M stars are powerful emitters of far-ultraviolet light. Over long timescales, a significant, possibly dominant, fraction of this emission is produced by stellar flares. Characteriz…
Stellar & Planetary Parameters for K2's Late Type Dwarf Systems from C1 to C5
Arturo O. Martinez, Ian J. M. Crossfield, Joshua E. Schlieder +12
The NASA K2 mission uses photometry to find planets transiting stars of various types. M dwarfs are of high interest since they host more short period planets than any other type o…
Predicting Lyman-alpha and Mg II Fluxes from K and M Dwarfs Using GALEX Ultraviolet Photometry
Evgenya L. Shkolnik, Kristina A. Rolph, Sarah Peacock +1
A star's UV emission can greatly affect the atmospheric chemistry and physical properties of closely orbiting planets with the potential for severe mass loss. In particular, the Ly…