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[ascl:1704.008] Transit: Radiative-transfer code for planetary atmospheres

Transit calculates the transmission or emission spectrum of a planetary atmosphere with application to extrasolar-planet transit and eclipse observations, respectively. It computes the spectra by solving the one-dimensional line-by-line radiative-transfer equation for an atmospheric model.

Code site:
https://github.com/exosports/transit
Appears in:
http://adsabs.harvard.edu/abs/2016arXiv160402692B
Bibcode:
2017ascl.soft04008C

ascl:1704.008
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