https://github.com/adrn/exoplanet
Fast & scalable MCMC for all your exoplanet needs!
Science Score: 10.0%
This score indicates how likely this project is to be science-related based on various indicators:
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○CITATION.cff file
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○codemeta.json file
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○.zenodo.json file
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○DOI references
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✓Academic publication links
Links to: arxiv.org, zenodo.org -
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○Institutional organization owner
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○JOSS paper metadata
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○Scientific vocabulary similarity
Low similarity (11.4%) to scientific vocabulary
Last synced: 10 months ago
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Repository
Fast & scalable MCMC for all your exoplanet needs!
Basic Info
- Host: GitHub
- Owner: adrn
- License: mit
- Default Branch: master
- Homepage: https://docs.exoplanet.codes
- Size: 74.5 MB
Statistics
- Stars: 0
- Watchers: 2
- Forks: 0
- Open Issues: 0
- Releases: 0
Fork of exoplanet-dev/exoplanet
Created about 6 years ago
· Last pushed about 6 years ago
https://github.com/adrn/exoplanet/blob/master/
# exoplanet _exoplanet_ is a toolkit for probabilistic modeling of transit and/or radial velocity observations of [exoplanets](https://en.wikipedia.org/wiki/Exoplanet) and other astronomical time series using [PyMC3](https://docs.pymc.io). _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 language to support many of the custom functions and distributions required when fitting exoplanet datasets. These features include: - A fast and robust solver for Kepler's equation. - Scalable Gaussian Processes using [celerite](https://celerite.readthedocs.io). - Fast and accurate limb darkened light curves using [starry](https://rodluger.github.io/starry). - Common reparameterizations for [limb darkening parameters](https://arxiv.org/abs/1308.0009), and [planet radius and impact parameter](https://arxiv.org/abs/1811.04859). - And many others! All of these functions and distributions include methods for efficiently calculating their _gradients_ so that they can be used with gradient-based inference methods like [Hamiltonian Monte Carlo](https://arxiv.org/abs/1206.1901), [No U-Turns Sampling](https://arxiv.org/abs/1111.4246), and [variational inference](https://arxiv.org/abs/1603.00788). These methods tend to be more robust than the methods more commonly used in astronomy (like [ensemble samplers](https://emcee.readthedocs.io) and [nested sampling](https://ccpforge.cse.rl.ac.uk/gf/project/multinest/)) especially when the model has more than a few parameters. For many exoplanet applications, _exoplanet_ (the code) can improve the typical performance by orders of magnitude. _exoplanet_ is being actively developed in [a public repository on GitHub](https://github.com/exoplanet-dev/exoplanet) so if you have any trouble, [open an issue](https://github.com/exoplanet-dev/exoplanet/issues) there.
Owner
- Name: Adrian Price-Whelan
- Login: adrn
- Kind: user
- Location: NYC
- Company: Flatiron Institute
- Website: adrian.pw
- Repositories: 124
- Profile: https://github.com/adrn