- Author
Patricio Cubillos and contributors (see
team)- Contact
- Organizations
- Web Site
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Pyrat Bay is an efficient, user-friendly tool to compute and fit radiative-transfer spectra. This package offers:
- Forward-model radiative-transfer calculation of:
- Transmission spectra (transit observations)
- Emission spectra (eclipse observations)
- Line-by-line calculation
- Opacity sources:
- Line-by-line molecular absorption
- Collision-induced absorption
- Rayleigh scattering absorption
- Na and K alkali resonant lines
- Gray and Mie scattering opacity
- Bayesian (MCMC) posterior sampling of atmospheric parameters:
- Molecular abundances
- Temperature profile
- Pressure-radius
- Rayleigh and cloud top levels
Note
Pyrat Bay is temporarily proprietary software. If you want to take a look before we release it, send me an email at patricio.cubillos[at]oeaw.ac.at.
- Patricio Cubillos (IWF) patricio.cubillos[at]oeaw.ac.at
- Jasmina Blecic (NYU Abu Dhabi)
- Joe Harrington (UCF)
getstarted tutorial lineread pyrat pyratbay units contributing license
- Please reference this paper if you found
Pyrat Bayuseful for your research: Cubillos et al. 2017: Yet Another Open-source Radiative-Transifer Code for Exoplanet Modeling, in preparation.
We welcome your feedback, but do not necessarily guarantee support. Please send feedback or inquiries to:
Patricio Cubillos (patricio.cubillos[at]oeaw.ac.at)
Pyrat-Bay is (temporarily) proprietary software (see license).
Note
It is imprtant to highlight that this project would not be possible without the previous experience with the BART project, nor without the contribution from each one of the collaborators to the BART code.
- Pyrat Bay version 0.0.50 (and earlier versions).