English

exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series

Instrumentation and Methods for Astrophysics 2021-06-25 v2 Earth and Planetary Astrophysics

Abstract

"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.

Keywords

Cite

@article{arxiv.2105.01994,
  title  = {exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series},
  author = {Daniel Foreman-Mackey and Rodrigo Luger and Eric Agol and Thomas Barclay and Luke G. Bouma and Timothy D. Brandt and Ian Czekala and Trevor J. David and Jiayin Dong and Emily A. Gilbert and Tyler A. Gordon and Christina Hedges and Daniel R. Hey and Brett M. Morris and Adrian M. Price-Whelan and Arjun B. Savel},
  journal= {arXiv preprint arXiv:2105.01994},
  year   = {2021}
}

Comments

Published in the Journal of Open Source Software. Comments (still) welcome. Software available at https://docs.exoplanet.codes

R2 v1 2026-06-24T01:47:53.271Z