13918

PyTransit: Fast and Easy Exoplanet Transit Modelling in Python

Hannu Parviainen
University of Oxford, Sub-Department of Astrophysics, Department of Physics, Oxford OX1 3RH
arXiv:1504.07433 [astro-ph.EP], (28 Apr 2015)

@article{parviainen2015pytransit,

   title={PyTransit: Fast and Easy Exoplanet Transit Modelling in Python},

   author={Parviainen, Hannu},

   year={2015},

   month={apr},

   archivePrefix={"arXiv"},

   primaryClass={astro-ph.EP},

   doi={10.1093/mnras/stv894}

}

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We present a fast and user friendly exoplanet transit light curve modelling package PyTransit, implementing optimised versions of the Gimen’ez and the Mandel & Agol transit models. The package offers an object-oriented Python interface to access the two models implemented natively in Fortran with OpenMP parallelisation. A partial OpenCL version of the quadratic Mandel-Agol model is also included for GPU-accelerated computations. The aim of PyTransit is to facilitate the analysis of photometric time series of exoplanet transits consisting of hundreds of thousands of datapoints, and of multi-passband transit light curves from spectrophotometric observations, as a part of a researcher’s programming toolkit for building complex, problem-specific, analyses.
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