Transit: Radiative-transfer code for planetary atmospheres
Abstract
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.
- Publication:
-
Astrophysics Source Code Library
- Pub Date:
- April 2017
- Bibcode:
- 2017ascl.soft04008C
- Keywords:
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- Software;
- NASA