activity
20242026
collaborators
Showing 2024Show all

7 papers · 1 filter

astro-ph.EP2024

History and Habitability of the LP 890-9 Planetary System

Rory Barnes, Laura N. R. do Amaral, Jessica Birky +42

We present numerous aspects of the evolution of the LP 890-9 (SPECULOOS-2/TOI-4306) planetary system, focusing on the likelihood that planet c can support life. We find that the ho…

astro-ph.EP2024

The TESS-Keck Survey. XXII. A sub-Neptune Orbiting TOI-1437

Daria Pidhorodetska, Emily A. Gilbert, Stephen R. Kane +40

Exoplanet discoveries have revealed a dramatic diversity of planet sizes across a vast array of orbital architectures. Sub-Neptunes are of particular interest; due to their absence…

astro-ph.HE2024

X-ray Emission of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones

Breanna A. Binder, Sarah Peacock, Edward W. Schwieterman +5

Stellar X-ray and UV radiation can significantly affect the survival, composition, and long-term evolution of the atmospheres of planets in or near their host star's habitable zone…

astro-ph.EP2024

A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

TRAPPIST-1 JWST Community Initiative, :, Julien de Wit +80

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most prominen…

astro-ph.EP2024

Artificial Greenhouse Gases as Exoplanet Technosignatures

Edward W. Schwieterman, Thomas J. Fauchez, Jacob Haqq-Misra +6

Atmospheric pollutants such as CFCs and NO have been proposed as potential remotely detectable atmospheric technosignature gases. Here we investigate the potential for artifi…

astro-ph.EP2024

The Impact of Extended HO Cross-Sections on Temperate Anoxic Planet Atmospheres: Implications for Spectral Characterization of Habitable Worlds

Wynter Broussard, Edward W. Schwieterman, Sukrit Ranjan +3

JWST has created a new era of terrestrial exoplanet atmospheric characterization, and with it the possibility to detect potential biosignature gases like CH. Our interpretati…