JWST spectra of young AB Dor L dwarfs show varying silicate absorption strengths, with 4/5 objects matching the trend of deeper features at equator-on inclinations and a tentative peak-wavelength correlation with viewing angle.
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High-resolution spectroscopy of 51 Peg b confirms atmospheric H2O, constrains high metallicity and solar C/O via Bayesian retrieval, and yields an alternative orbital semi-amplitude of 102.8 km/s with revised mass 0.61 MJup and inclination 49.8 deg.
citing papers explorer
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Clouds with a silicate lining: Using JWST spectra to probe atmospheric diversity in young AB Dor L dwarfs
JWST spectra of young AB Dor L dwarfs show varying silicate absorption strengths, with 4/5 objects matching the trend of deeper features at equator-on inclinations and a tentative peak-wavelength correlation with viewing angle.
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51 Peg b revisited with VLT/CRIRES+. Constraints on atmospheric thermal structure, chemical composition, and an alternative orbital solution
High-resolution spectroscopy of 51 Peg b confirms atmospheric H2O, constrains high metallicity and solar C/O via Bayesian retrieval, and yields an alternative orbital semi-amplitude of 102.8 km/s with revised mass 0.61 MJup and inclination 49.8 deg.