High-resolution spectroscopic detection of reflected light from LTT-9779 b at SNR 5.4 giving Fp/F* = 102 ppm and Ag = 0.88 assuming Lambertian scattering.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
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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High-resolution detection of reflected light from the exo-Neptune LTT-9779 b
High-resolution spectroscopic detection of reflected light from LTT-9779 b at SNR 5.4 giving Fp/F* = 102 ppm and Ag = 0.88 assuming Lambertian scattering.
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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.