Tentative CO detection from WASP-33b eclipse data alone with SPIRou validates stacking ingresses/egresses and shows Doppler eclipse mapping can constrain rotation with additional observations.
, archivePrefix = "arXiv", eprint =
5 Pith papers cite this work. Polarity classification is still indexing.
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2026 5verdicts
UNVERDICTED 5representative citing papers
MOSES is a vacuum-stabilized white-pupil echelle spectrograph designed for >80,000 resolution over 380-680 nm and sub-2 m/s RV precision via dual-fiber simultaneous Fabry-Pérot calibration on the MONET telescope.
Designs for two Fabry-Pérot etalons (15 GHz and 12.2 GHz FSR) and associated Th-Ne/U-Ar/U-Ne calibration units are presented for CARMENES, claiming internal stability better than 10 cm/s per night with thousands of reference lines.
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.
Describes a fiber-coupling setup for Bruker IFS 125 FTS with hexagonal fibers for mode scrambling and dichroic combining for dual-source measurements.
citing papers explorer
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Towards Doppler eclipse mapping of hot Jupiters. An observational perspective on WASP-33 b with SPIRou
Tentative CO detection from WASP-33b eclipse data alone with SPIRou validates stacking ingresses/egresses and shows Doppler eclipse mapping can constrain rotation with additional observations.
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MOSES -- The MONET Star and Exoplanet Spectrograph
MOSES is a vacuum-stabilized white-pupil echelle spectrograph designed for >80,000 resolution over 380-680 nm and sub-2 m/s RV precision via dual-fiber simultaneous Fabry-Pérot calibration on the MONET telescope.
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Two Fabry-Perots and two calibration units for CARMENES
Designs for two Fabry-Pérot etalons (15 GHz and 12.2 GHz FSR) and associated Th-Ne/U-Ar/U-Ne calibration units are presented for CARMENES, claiming internal stability better than 10 cm/s per night with thousands of reference lines.
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The Pan-Pacific Planet Search -- IX. A menagerie of companions orbiting evolved stars
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.
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Fiber-coupling of Fourier Transform Spectrographs
Describes a fiber-coupling setup for Bruker IFS 125 FTS with hexagonal fibers for mode scrambling and dichroic combining for dual-source measurements.