collaborators

7 papers

astro-ph.EP2026

KRONOS I: The m JWST Transmission Spectrum of the 23 Myr V1298 Tau c

Matthew M. Murphy, Matthew C. Nixon, Adina D. Feinstein +16

While recent JWST observations of mature super-Earths and sub-Neptunes have frequently revealed featureless transmission spectra, their inflated progenitors offer a unique window i…

astro-ph.SR2026

KRONOS II: Solar-like Umbra and Penumbra Properties on the Young Sun V1298~Tau

Matthew M. Murphy, Adina D. Feinstein, Meir E. Schochet +14

Transiting exoplanets provide a unique laboratory for studying stellar surface heterogeneities via starspot or facular occultations. When observed at multiple wavelengths, this con…

astro-ph.EP2026

A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884

C. A. Murray, L. Garcia, B. V. Rackham +18

TOI-3884 b is a rare super-Neptune transiting a fully convective M dwarf that hosts a persistent giant polar spot. Because the planet occults this active region during every transi…

astro-ph.EP2026

Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves

C. A. Murray, Z. Berta-Thompson

Starspot-crossing events (SCEs) in exoplanet transit lightcurves are becoming increasingly common as we focus on cooler host stars and observe higher precision photometric and spec…

astro-ph.EP2026

The 3D Cosmic Shoreline for Nurturing Planetary Atmospheres

Zach K. Berta-Thompson, Patcharapol Wachiraphan, Catriona Murray

Various ``cosmic shorelines" have been proposed to delineate which planets have atmospheres. The fates of individual planet atmospheres may be set by a complex sea of growth and lo…

astro-ph.IM2025

exoatlas: friendly Python code for exoplanet populations

Zach K. Berta-Thompson, Patcharapol Wachiraphan, Autumn Stephens +6

Planets are complicated. Understanding how they work requires connecting individual objects to the context of broader populations. Exoplanets are easier to picture next to their cl…