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[ascl:1810.005] STARRY: Analytic computation of occultation light curves

STARRY computes light curves for various applications in astronomy: transits and secondary eclipses of exoplanets, light curves of eclipsing binaries, rotational phase curves of exoplanets, light curves of planet-planet and planet-moon occultations, and more. By modeling celestial body surface maps as sums of spherical harmonics, STARRY does all this analytically and is therefore fast, stable, and differentiable. Coded in C++ but wrapped in Python, STARRY is easy to install and use.

Code site:
https://github.com/rodluger/starry https://rodluger.github.io/starry/
Appears in:
http://adsabs.harvard.edu/abs/2018arXiv181006559L
Bibcode:
2018ascl.soft10005L

Views: 90

ascl:1810.005
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