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20182021
most citedImproved Constraints for the XUV Luminosity Evolution of Trappist-1

19 citations · 30 across the 3 of their papers we have counts for

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astro-ph.EP202119 cited

Improved Constraints for the XUV Luminosity Evolution of Trappist-1

Jessica Birky, Rory Barnes, David P. Fleming

We re-examine the XUV luminosity evolution of TRAPPIST-1 utilizing new observational constraints (XUV and bolometric luminosity) from multi-epoch X-ray/UV photometry. Following the…

astro-ph.EP2020

Orbital evolution of potentially habitable planets of tidally interacting binary stars

David E. Graham, David P. Fleming, Rory Barnes

We simulate the coupled stellar and tidal evolution of short-period binary stars (orbital period $P_{orb} \lsim$8 days) to investigate the orbital oscillations, instellation cycles…

astro-ph.EP2019

VPLanet: The Virtual Planet Simulator

Rory Barnes, Rodrigo Luger, Russell Deitrick +14

We describe a software package called VPLanet that simulates fundamental aspects of planetary system evolution over Gyr timescales, with a focus on investigating habitable worlds.…

astro-ph.EP20197 cited

A Statistical Comparative Planetology Approach to Maximize the Scientific Return of Future Exoplanet Characterization Efforts

Jade H. Checlair, Dorian S. Abbot, Robert J. Webber +37

Provided that sufficient resources are deployed, we can look forward to an extraordinary future in which we will characterize potentially habitable planets. Until now, we have had…

astro-ph.EP20194 cited

The Importance of 3D General Circulation Models for Characterizing the Climate and Habitability of Terrestrial Extrasolar Planets

Eric T. Wolf, Ravi Kopparapu, Vladimir Airapetian +27

While recently discovered exotic new planet-types have both challenged our imaginations and broadened our knowledge of planetary system workings, perhaps the most compelling object…

astro-ph.EP2018

Exo-Milankovitch Cycles II: Climates of G-dwarf Planets in Dynamically Hot Systems

Russell Deitrick, Rory Barnes, Cecilia Bitz +6

Using an energy balance model with ice sheets, we examine the climate response of an Earth-like planet orbiting a G dwarf star and experiencing large orbital and obliquity variatio…