Non-detection of CH4 and CO fluorescence in JWST spectra sets upper limits on their surface partial pressures at (3-10)×10^{-6} and (50-300)×10^{-6} nbar, well below the 100-200 nbar total pressure from occultation data.
A., Bertrand, T., Trafton, L
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Constraints on the Atmospheric Composition of 2002 XV$_{93}$ from JWST Spectroscopy
Non-detection of CH4 and CO fluorescence in JWST spectra sets upper limits on their surface partial pressures at (3-10)×10^{-6} and (50-300)×10^{-6} nbar, well below the 100-200 nbar total pressure from occultation data.