Exomod: A Python Library for Exoplanet Transit Light Curve Fitting and Stacking with Background Simulation and Optimization

From the light curve taken during exoplanet transit, important parameters such as the radius ratio of the star-planet, impact parameter, inclination, and relative tangential velocity could be derived. A module was developed in the form of a Python library based on modeling using background simulatio...

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Veröffentlicht in:Journal of physics. Conference series Jg. 2866; H. 1; S. 12064 - 12075
Hauptverfasser: Akilah, Rafa Nanda, Randolph, Bryant, Khawariz Andaristiyan, M.
Format: Journal Article
Sprache:Englisch
Veröffentlicht: Bristol IOP Publishing 01.10.2024
Schlagworte:
Curve fitting
Evolutionary computation
Extrasolar planets
Impact analysis
Light curve
Limb darkening
Local optimization
Parameters
Transit
ISSN:1742-6588, 1742-6596
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Zusammenfassung:From the light curve taken during exoplanet transit, important parameters such as the radius ratio of the star-planet, impact parameter, inclination, and relative tangential velocity could be derived. A module was developed in the form of a Python library based on modeling using background simulation and fitting by utilizing global and local optimization, such as differential evolution and the Broyden–Fletcher–Goldfarb–Shanno (BFGS) method. For more accurate fitting, the effects of linear limb darkening on exoplanets are also included. The performance testing for the program was done by using dummy data to test its accuracy, followed by validation tests using WASP-12b transit curves to find out any discrepancies between our model and real exoplanet data. While performing a characterization test on WASP-12b, we found an interesting result regarding its impact parameter and the exoplanet’s velocity, which might be an interesting subject for further analysis.
Bibliographie:ObjectType-Article-1
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ISSN:1742-6588
1742-6596
DOI:10.1088/1742-6596/2866/1/012064