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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No exomoon signal detected in radial velocity data of β Pictoris b; upper limits reach 80 Earth masses at 1-day periods and 1 Jupiter mass at 200-day periods.
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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Upper limits on exosatellites around $\beta$ Pictoris b
No exomoon signal detected in radial velocity data of β Pictoris b; upper limits reach 80 Earth masses at 1-day periods and 1 Jupiter mass at 200-day periods.