works on

From the 1 of 13 linked papers with an AI index.

activity
20242026
collaborators

13 papers

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

Native-resolution retrievals of VHS 1256-1257 b spanning the JWST/NIRSpec wavelength range: Chemical composition of a partially cloudy atmosphere

S. de Regt, N. Whiteford, B. E. Miles +3

The wide wavelength coverage and sensitivity offered by JWST enable detailed analyses of extrasolar atmospheres. At its highest resolution (R~2700), NIRSpec measures the absorption…

astro-ph.EP2026

The ESO SupJup Survey XI. Atmospheric properties of six isolated M- and L-type dwarfs with CRIRES+

C. R. Malcolm, N. Grasser, I. A. G. Snellen +9

The distinct formation pathways of brown dwarfs and giant exoplanets may be encoded in their atmospheric composition. We present atmospheric retrievals for six isolated brown dwarf…

astro-ph.EP2026

The carbon isotope ratio of β Pic b with high-resolution spectroscopy

D. González Picos, I. A. G. Snellen, R. Landman +6

Isotopic ratios trace the formation and evolution of planets and link their atmospheres to the chemistry of their natal protoplanetary discs. We measure $^{12}\mathrm{C}/^{13}\math…

astro-ph.EP2026

Strong and variable stratospheric CO emission from lava-planet 55 Cnc e observed with NIRCam/JWST

Ignas Snellen, Yamila Miguel, Leoni Janssen +4

Some rocky planets orbit so close to their host stars that stellar heating melts their surfaces. They offer a rare glimpse of planets in a magma-ocean state, providing an observabl…

astro-ph.EP2026

The ESO SupJup Survey. X. A carbon isotope contrast in the young ROXs 12 system

N. Grasser, I. A. G. Snellen, S. de Regt +7

Emerging research suggests that elemental and isotopic ratios of exoplanet and brown dwarf atmospheres may serve as potential tracers of their formation pathways. The ESO SupJup Su…