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20242026
most citedDetecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet

4 citations · 7 across the 12 of their papers we have counts for

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astro-ph.SR2025

X-ray and UV Observations of the Young Sun HIP~67522: Evidence of Lyman-alpha Absorption Within the Planetary System

Cynthia S. Froning, Allison Youngblood, David J. Wilson +7

We present ultraviolet (UV) spectroscopy of the 17 Myr, G0V star, HIP 67522. The UV spectrum is characterized by strong chromospheric and transition region emission lines. There wa…

astro-ph.SR2025

Lyman-Alpha Emission from K and M Dwarfs: Intrinsic Profiles, Variability, and Flux in the Habitable Zone

Sarah Peacock, Travis S. Barman, R. O. Parke Loyd +4

Lyman- (Ly) is the most prominent ultraviolet emission line in low-mass stars, playing a crucial role in exoplanet atmospheric photochemistry, heating, and escape. However, i…

astro-ph.SR2025

HWO Target Stars and Systems: A Survey of Archival UV and X-ray Data

Sarah Peacock, David J. Wilson, Tyler Richey-Yowell +14

We assess archival high-energy data for key stars on the Habitable Worlds Observatory (HWO) Target Stars and Systems 2025 list, as stellar radiation is critical to shaping and inte…

astro-ph.SR2025

Toward a 2D H I Map of the Local Interstellar Medium

Allison Youngblood, Kevin France, Tommi Koskinen +9

Obtaining a complete census of gas in the local interstellar medium (<100 pc) is challenging given the limited available tracers of the warm, partially-ionized medium. Medium-to-hi…

astro-ph.SR2025★ 4 cited

Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet

James Paul Mason, Allison Youngblood, Kevin France +2

Stellar flares and coronal mass ejections (CMEs) can strip planetary atmospheres, reducing the potential habitability of terrestrial planets. While flares have been observed for de…

astro-ph.SR2025

A Semi-Empirical Estimate of Solar EUV Evolution from 10 Myr to 10 Gyr

Kevin France, Girish Duvvuri, Cynthia Froning +9

The extreme-ultraviolet (EUV; 100 -- 911 Å) spectra of F, G, K, and M stars provide diagnostics of the stellar chromosphere through the corona, with line and continuum formation te…