Updated RM modeling framework in TLCM validated on nine systems and applied to TOI-135 to measure sky-projected obliquity λ = 55.6° with ~11° uncertainties.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Giant planets around stars in binaries are more massive, orbit closer in, and appear more inflated than those around single stars, with a tentative excess around M-dwarfs in systems closer than 1000 AU.
citing papers explorer
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A comprehensive Rossiter-Mclaughlin Modelling Framework in TLCM: Application to HD 2685 $=$ TOI-135 system
Updated RM modeling framework in TLCM validated on nine systems and applied to TOI-135 to measure sky-projected obliquity λ = 55.6° with ~11° uncertainties.
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Mind the Companion : Demographics of Transiting S-type Exoplanets
Giant planets around stars in binaries are more massive, orbit closer in, and appear more inflated than those around single stars, with a tentative excess around M-dwarfs in systems closer than 1000 AU.