Radial velocity measurements of the brown dwarf CD-35 2722 B reveal a strong 169-day periodic signal attributed to a ~0.74 Jupiter-mass satellite, with a weaker secondary signal possibly indicating a second satellite near 2:1 resonance.
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6 Pith papers cite this work, alongside 84 external citations. Polarity classification is still indexing.
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2026 6representative citing papers
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.
The paper outlines a staged observational campaign with the Nautilus Space Observatory for astrometric detection of exomoons around nearby imaged exoplanets.
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.
JWST/MIRI imaging of Eps Ind A b prefers a double-PSF model likely due to systematics but demonstrates sensitivity to exomoons down to 1.3 M_Jup at separations >2 AU and 2.5 M_Jup at 0.52 AU.
CARMApy provides a Python interface to the ExoCARMA microphysics code, enabling simulation of cloud particle size distributions and rates in exoplanet atmospheres with claimed consistency to prior versions and speed gains of 1.9x single-threaded and 3.8x multithreaded.
citing papers explorer
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Planetary-Mass Exosatellite Detected Around the Substellar Companion of a Star
Radial velocity measurements of the brown dwarf CD-35 2722 B reveal a strong 169-day periodic signal attributed to a ~0.74 Jupiter-mass satellite, with a weaker secondary signal possibly indicating a second satellite near 2:1 resonance.
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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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A Scalable Path to Astrometric Exomoon Discoveries with the Nautilus Space Observatory
The paper outlines a staged observational campaign with the Nautilus Space Observatory for astrometric detection of exomoons around nearby imaged exoplanets.
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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.
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Direct Imaging Constraints on Binary Planets and Exomoons around Epsilon Indi A b
JWST/MIRI imaging of Eps Ind A b prefers a double-PSF model likely due to systematics but demonstrates sensitivity to exomoons down to 1.3 M_Jup at separations >2 AU and 2.5 M_Jup at 0.52 AU.
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CARMApy: An Open-Source Python Framework for Simulating Microphysical Clouds in Planetary Atmospheres
CARMApy provides a Python interface to the ExoCARMA microphysics code, enabling simulation of cloud particle size distributions and rates in exoplanet atmospheres with claimed consistency to prior versions and speed gains of 1.9x single-threaded and 3.8x multithreaded.