Catwoman: A transit modelling Python package for asymmetric light curves
When exoplanets pass in front of their stars, they imprint a transit signature on the stellar light curve which to date has been assumed to be symmetric in time, owing to the planet being modelled as a circular area occulting the stellar surface. However, this signature might be asymmetric due to di...
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          | Published in | arXiv.org | 
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| Main Authors | , | 
| Format | Paper Journal Article | 
| Language | English | 
| Published | 
        Ithaca
          Cornell University Library, arXiv.org
    
        29.06.2021
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| Subjects | |
| Online Access | Get full text | 
| ISSN | 2331-8422 | 
| DOI | 10.48550/arxiv.2106.15643 | 
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| Summary: | When exoplanets pass in front of their stars, they imprint a transit signature on the stellar light curve which to date has been assumed to be symmetric in time, owing to the planet being modelled as a circular area occulting the stellar surface. However, this signature might be asymmetric due to different temperature/pressure and/or chemical compositions in the different terminator regions of the transiting planet. catwoman is a Python package that allows to model these asymmetric transit lightcurves, calculating lightcurves for any radially symmetric stellar limb darkening law, and where planets are modelled as two semi-circles, of different radii, using the integration algorithm developed in arXiv:1507.08285 and implemented in the batman library, from which catwoman builds upon. | 
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| Bibliography: | SourceType-Working Papers-1 ObjectType-Working Paper/Pre-Print-1 content type line 50  | 
| ISSN: | 2331-8422 | 
| DOI: | 10.48550/arxiv.2106.15643 |