collaborators

13 papers

astro-ph.EP2026

Leveraging Impact Parameter to Mitigate the Transit Light Source Effect: Early Insights from TRAPPIST-1

Ana Glidden, Alexander I. Shapiro, Sara Seager +19

Stellar activity complicates exoplanet transmission spectra, particularly for smaller planets around M dwarfs with JWST. The transit light source (TLS) effect, the imprinting of sp…

astro-ph.IM2026

Mapping Stellar Heterogeneities with the Nautilus Space Observatory

Adina D. Feinstein, Jeff Valenti, Julien de Wit +9

Stellar photospheric heterogeneities, such as starspots and faculae, are a fundamental limitation for exoplanet transmission spectroscopy. Inhomogeneous surfaces can imprint wavele…

astro-ph.SR2026

Nautilus: Fast Time-Resolved Spectroscopy of GKM Stellar Flares and Their Implications for Planetary Habitability

Chia-Lung Lin, Adina D. Feinstein, Jeff Valenti +10

Low-mass GKM dwarfs are prime targets for finding habitable-zone Earth-sized planets, but their frequent flares, especially on M~dwarfs, can strongly affect planetary atmospheres t…

physics.chem-ph2026

Comprehensive Ab Initio Quantum Computations of CO-H and CO-He Collisional Properties

Prajwal Niraula, Laurent Wiesenfeld, Nejmeddine Jaïdane +6

We present comprehensive \textsl{ab initio} fully quantum calculations of CO--H and CO--He collisional properties. Our framework combines CCSD(T) pote…

astro-ph.SR2026

Unlocking HST's Stellar Treasure Trove: Stellar Activity Minima for HAT-P-11 Offer Prime Windows for Transmission Spectroscopy

Prajwal Niraula, Benjamin V. Rackham, Julien de Wit +4

HAT-P-11 is a well-studied, active K dwarf hosting an eccentric, misaligned transiting sub-Neptune. As part of the HST Stellar Treasure Trove program (HST-AR-17551), we analyze abs…

astro-ph.EP2026

Helium Atmospheres May Hide in Current Exoplanet Analysis Frameworks

Julien de Wit, Aaron Householder, Prajwal Niraula

The increasing number of detailed exoplanet observations offers an opportunity to refine our analyses and interpretations. Here, we show that atmospheres that appear volatile-rich…