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exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series
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"exoplanet" is a toolkit for probabilistic modeling of astronomical time series data, with a focus on observations of exoplanets, using PyMC3 (Salvatier et al., 2016). PyMC3 is a flexible and high-performance model-building language and inference engine that scales well to problems with a large number of parameters. "exoplanet" extends PyMC3's modeling language to support many of the custom functions and probability distributions required when fitting exoplanet datasets or other astronomical time series. While it has been used for other applications, such as the study of stellar variability, the primary purpose of "exoplanet" is the characterization of exoplanets or multiple star systems using time-series photometry, astrometry, and/or radial velocity. In particular, the typical use case would be to use one or more of these datasets to place constraints on the physical and orbital parameters of the system, such as planet mass or orbital period, while simultaneously taking into account the effects of stellar variability.
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Cited by 3 Pith papers
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Revisiting TOI-4438 and TOI-442 planetary systems with new observations from SPIRou and TESS
Refined masses and radii for TOI-4438 b and TOI-442 b, stellar rotation periods from magnetic variability, and a single-transit planet candidate around TOI-4438.
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Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation
Homogeneous SpeX metallicities of M-dwarf planet hosts show sub-Neptune hosts are more metal-rich than super-Earth hosts, supporting ice-line formation plus migration.
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An Aligned Sub-Neptune Revealed with MAROON-X and a Tendency Towards Alignment for Small Planets
The sub-Neptune TOI-1759A b has sky-projected obliquity |λ|=4±18 deg, and small exoplanets with measured obliquities tend toward alignment, especially in compact systems.
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