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From the 2 of 8 linked papers with an AI index.

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8 papers

astro-ph.IM2026

ForMoSA: Forward Modeling tool for Spectral Analysis

ForMoSA Collaboration, Simon Petrus, Paulina Palma-Bifani +9

ForMoSA is an open‑source Python package that uses Bayesian methods to fit spectroscopic and photometric data of directly imaged young planetary‑mass brown dwarfs and exoplanets, s…

astro-ph.EP2026

Latitudinal chemical and cloud variations in the atmosphere of a brown dwarf

Benjamin Charnay, Sam de Regt, Matthieu Ravet +8

The paper introduces a technique called Differential Molecular Rotational Broadening to detect latitudinal chemical differences in brown dwarf atmospheres, and applies it to VLT-CR…

astro-ph.EP2026

Next-generation Exo-REM atmospheric models: application to VHS 1256 b to emulate patchy clouds

Alice Radcliffe, Benjamin Charnay, Anne-Marie Lagrange +7

Condensate clouds are a defining feature of brown dwarf and exoplanet atmospheres, producing a broad range of colours on the CMD and giving rise to spectral features such as the di…

astro-ph.EP2026

Panchromatic View of the Frigid Jovian Exoplanet COCONUTS-2 b

Matthieu Ravet, Mickaël Bonnefoy, Gaël Chauvin +24

We use a high signal-to-noise MIRI-LRS spectrum (5.45 - 11 m, R ) of COCONUTS-2~b revealing prominent molecular features of HO, CH and NH. This datase…

astro-ph.EP2026

Cold and eccentric: a high-spectral resolution view of 51 Eri b with VLT/HiRISE

A. Denis, A. Vigan, G. Chauvin +35

Discovered almost 10 years ago, the giant planet 51 Eridani b is one of the least separated (0.2 arcsec) and faintest (J = 19.74 mag) directly imaged exoplanets known to date. Its…

astro-ph.EP2025

GPI+SPHERE detection of a 6.1 circumbinary planet around HD 143811

Vito Squicciarini, Johan Mazoyer, Christian Wilkinson +6

Owing to its sensitivity to wide-orbit giant exoplanets, direct imaging is uniquely positioned to shed light on the interplay between protoplanetary disks and stellar hosts. In add…