most citedEvidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b

2 citations · 2 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph.EP20262 cited

Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b

Brandon Park Coy, Qiao Xue, Megan Weiner Mansfield +14

'Lava worlds'-Earth-sized planets hot enough (Teq >~ 1100 K) to melt their dayside silicate surfaces-have emerged as promising candidates for atmospheric detection and characteriza…

astro-ph.EP2026

Magnetic field strengths of hot giant exoplanets consistent with Solar System values

Julia V. Seidel, Vivien Parmentier, Bibiana Prinoth +29

Magnetic fields are ubiquitous in the universe. They play a key role in shaping the activity of stars, the habitability of rocky planets, and the long-term retention of planetary a…

astro-ph.EP2026

Reinterpreting the JWST Observations of 55 Cancri e with a Non-Grey General Circulation Model

Ruizhi Zhan, Daniel D. B. Koll

Recent observations of 55 Cancri e suggest an atmosphere rich in CO or CO (Hu et al. 2024); other observations indicate the planet's eclipse depth is highly variable (e.g. Pate…

astro-ph.EP2026

The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy

Sebastian Zieba, Laura Kreidberg, Brandon P. Coy +13

JWST has opened a new era in the study of rocky exoplanets, enabling direct characterization of their surfaces with mid-infrared spectroscopy. Different types of rock have distinct…

astro-ph.EP2025

Bistability, Oscillations, and Multistability on Hycean Planets

Yichen Gao, Daniel D. B. Koll, Feng Ding

Hycean planets are hypothetical exoplanets characterized by oceans and -rich atmospheres. These planets are high-priority targets for biosignature searches, as they com…

astro-ph.EP2025

Impact of Subsurface Temperature Gradients on Emission Spectra of Airless Exoplanets: the Solid-state Greenhouse and Anti-Greenhouse

Xintong Lyu, Daniel D. B. Koll

An emerging goal of exoplanet science is to constrain the surface composition of airless exoplanets. Without the protection of an atmosphere, these planets are likely covered by a…