collaborators

6 papers

astro-ph.EP2025

Inferring and Interpreting the Visual Geometric Albedo and Phase Function of Earth

Tyler D. Robinson

Understanding reflectance-related quantities for worlds enables effective comparative planetology and strengthens mission planning and execution. Measurements of these properties f…

astro-ph.EP2025

The Open-Source Photochem Code: A General Chemical and Climate Model for Interpreting (Exo)Planet Observations

Nicholas F. Wogan, Natasha E. Batalha, Kevin Zahnle +7

With the launch of the James Webb Space Telescope, we are firmly in the era of exoplanet atmosphere characterization. Understanding exoplanet spectra requires atmospheric chemical…

astro-ph.EP2025

Extreme Forward Scattering Observed in Disk-Averaged Near-Infrared Phase Curves of Titan

Chase A. Cooper, Tyler D. Robinson, Jason W. Barnes +2

Titan, with its thick and hazy atmosphere, is a key world in our solar system for understanding light scattering processes. NASA's Cassini mission monitored Titan between 2004 and…

astro-ph.EP2025

Modern Earth-like Chemical Disequilibrium Biosignatures Are Challenging To Constrain Through Spectroscopic Retrievals

Amber Young, Tyler Robinson, Joshua Krissansen-Totton +4

Robust exoplanet characterization studies are underway, and the community is looking ahead toward developing observational strategies to search for life beyond our solar system. Wi…

astro-ph.EP2024

Potential technosignature from anomalously low deuterium/hydrogen (D/H) in planetary water depleted by nuclear fusion technology

David C. Catling, Joshua Krissansen-Totton, Tyler D. Robinson

Deuterium-deuterium (DD) fusion is viewed as an ideal energy source for humanity in the far future, given a vast seawater supply of D. Here, we consider long-lived, extraterrestria…

astro-ph.EP2024

Microphysical Prescriptions for Parameterized Water Cloud Formation on Ultra-cool Substellar Objects

James Mang, Caroline V. Morley, Tyler D. Robinson +1

Water must condense into ice clouds in the coldest brown dwarfs and exoplanets. When they form, these icy clouds change the emergent spectra, temperature structure, and albedo of t…