works on

From the 1 of 8 linked papers with an AI index.

activity
20242026
collaborators

8 papers

astro-ph.EP2026

The JWST weather report: Unravelling the atmospheric variability of isolated worlds using principal component analysis

Merle A. Schrader, Johanna M. Vos, Evert Nasedkin +17

The paper uses principal component analysis on JWST/NIRSpec time‑series spectra of the brown dwarf SIMP‑0136 to identify two dominant patterns of variability, linking them to tempe…

astro-ph.EP2026

Assessing Ariel's capabilities to observe free-floating brown dwarfs

Roman Akhmetshyn, Nicolas B Cowan, Sarah Casewell

The primary goal of the Ariel space telescope is to conduct the biggest spectroscopic survey of transiting exoplanets to characterize their atmospheres and weather. We propose to e…

astro-ph.EP2026

Coupled orbital and interior structure evolution of lava planets

Mahesh Herath, Nicolas B. Cowan, Charles-Édouard Boukaré +1

Lava planets likely did not form in their current orbits, instead migrating inward via orbital decay, which influenced the evolution of their magma oceans. We introduce a coupled t…

astro-ph.EP2026

Mapping the Cloud-Driven Atmospheric Dynamics & Chemistry of an Isolated Exoplanet Analog with Harmonic Signatures

Michael K. Plummer, Francis P. Cocchini, Peter A. Kearns +12

Young planetary-mass objects and brown dwarfs near the L/T spectral transition exhibit enhanced spectrophotometric variability over field brown dwarfs. Patchy clouds, auroral proce…

astro-ph.EP2025

Rock vapour is opaque: implications for dynamics and observations of lava planets

T. Giang Nguyen, Nicolas B. Cowan, Gunnar Montseny Gens +3

Extreme instellation on lava planets causes the rocky surface to melt and vaporize. Because the rock vapour composition is intrinsically tied to the mantle, atmospheric characteriz…

astro-ph.EP2025

Heat Reveals What Clouds Conceal: Global Carbon & Longitudinally Asymmetric Chemistry on LTT 9779 b

Reza Ashtari, Sean Collins, Jared Splinter +17

LTT-9779 b is an ultra-hot Neptune (Rp ~ 4.7 Re, Mp ~ 29 Me) orbiting its Sun-like host star in just 19 hours, placing it deep within the "hot Neptune desert," where Neptunian plan…