https://github.com/sevenian3/ChromaStarPy
Revision 8756752fe08fe8ee8d36574c02164b7e0f2d6b87 authored by Ian Short on 11 June 2021, 18:11:36 UTC, committed by GitHub on 11 June 2021, 18:11:36 UTC
Updated README and Input.py sample and minor improvements to administration of exoplanet transit lightcurve. Code no longer crashes when ifTransit is False
1 parent 441f211
Tip revision: 8756752fe08fe8ee8d36574c02164b7e0f2d6b87 authored by Ian Short on 11 June 2021, 18:11:36 UTC
Minor lightcurve improvements
Minor lightcurve improvements
Tip revision: 8756752
README.md
# ChromaStarPy
python stellar atmosphere and spectrum modeling code
A python3 code to compute the vertial structure of a static, plane-parallel, one-dimensional stellar atmosphere in local thermodynamic
equilibrium (LTE), and to compute the emergent spectrum incorporating opacity computed with a comprehensive atomic line list from
the NIST Atomic Spectra Database (https://www.nist.gov/pml/atomic-spectra-database) (Kramida, A., Ralchenko, Y., and Reader, J.,
and the NIST team, NIST Atomic Spectra Database ver 5.3, National Institute of Standards and Technology, Gaithersburg, Md.).
Provides post-processed data products that are ready to visualize in a python IDE such as spyder.
Useful for senior undergrads in astronomy and physics to experiment with and develop a stellar astrophysical modeling code in a graphical
IDE, and to compare observational data to ad hoc model output.
This is a port of the Java ChromaStarServer code (see GrayStar github repository) and will be kept synced with it.
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