ASCL Code Record
[ascl:2411.030]
NEMESISPY: Modeling exoplanet spectra
NEMESISPY infers the atmospheric properties of exoplanets, such as chemical composition, using spectroscopic data. The package calculates radiative transfer using the correlated-k approximation and for parametric atmospheric modelling. NEMESISPY is a Python implementation of the well-established Fortran NEMESIS library (ascl:2210.009), which has been applied to the atmospheric retrievals of both solar system planets and exoplanets employing numerous different observing geometries.
- Code site:
- https://github.com/Jingxuan97/nemesispy
- Used in:
- https://ui.adsabs.harvard.edu/abs/2023MNRAS.525.5146Y https://ui.adsabs.harvard.edu/abs/2024ApJ...975L..11B
- Described in:
- https://ui.adsabs.harvard.edu/abs/2024JOSS....9.6874Y
- EMAC link:
- https://emac.gsfc.nasa.gov/?cid=2409-001
- Bibcode:
- 2024ascl.soft11030Y
