activity
20212026
most citedThe fundamentals of Lyman-alpha exoplanet transits

42 citations · 82 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

Observational Signatures of Circumstellar Gas Tori Formed by Planetary Mass-Loss from Close-In Exoplanets

Ethan Schreyer, Ruth Murray-Clay

Close-in exoplanets with H/He atmospheres often undergo hydrodynamic escape. In extreme cases, it is hypothesized that the mass loss can be high enough for the escaping planetary m…

astro-ph.EP2026

Using observations of escaping H/He to constrain the atmospheric composition of sub-Neptunes

James G. Rogers, James E. Owen, Ethan Schreyer +1

The internal composition of sub-Neptunes remains a prominent unresolved question in exoplanetary science. We present a technique to place constraints on envelope mean molecular wei…

astro-ph.EP2025

The First Dedicated Survey of Atmospheric Escape from Planets Orbiting F Stars

Morgan Saidel, Shreyas Vissapragada, Heather Knutson +9

Hydrodynamic escape can strip the envelopes of close-in exoplanets, but most observations of atmospheric mass loss to date have been confined to planets orbiting K and M dwarfs. A…

astro-ph.EP2023★ 12 cited

Using Lyman- transits to constrain models of atmospheric escape

Ethan Schreyer, James. E. Owen, R. O. Parke Loyd +1

Lyman- transits provide an opportunity to test models of atmospheric escape directly. However, translating observations into constraints on the properties of the escaping atmosp…

astro-ph.EP2023★ 28 cited

Using helium 10830 Å transits to constrain planetary magnetic fields

Ethan Schreyer, James E. Owen, Jessica J. Spake +2

Planetary magnetic fields can affect the predicted mass loss rate for close-in planets that experience large amounts of UV irradiation. In this work, we present a method to detect…

astro-ph.EP2021★ 42 cited

The fundamentals of Lyman-alpha exoplanet transits

James E. Owen, Ruth A. Murray-Clay, Ethan Schreyer +7

Lyman- transits have been detected from several nearby exoplanets and are one of our best insights into the atmospheric escape process. However, due to ISM absorption, we typica…