BeyonCE -- Light Curve Modelling Beyond Circular Eclipsers I. Shallot Explorer

Context. Time-series photometry has given astronomers the tools to study time-dependent astrophysical phenomena, from stellar activity to fast radio bursts and exoplanet transits. Transit events in particular are focused primarily on planetary transits, and eclipsing binaries with eclipse geometries...

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Bibliographic Details
Published in:arXiv.org 2024-04
Main Authors: Dirk van Dam, Kenworthy, Matthew
Format: Article
Language:English
Subjects:
Celestial bodies
Complex variables
Depth profiling
Eclipsing binary stars
Extrasolar planets
Light curve
Optical thickness
Parameters
Radio bursts
Stellar activity
Time dependence
Transit
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Summary:Context. Time-series photometry has given astronomers the tools to study time-dependent astrophysical phenomena, from stellar activity to fast radio bursts and exoplanet transits. Transit events in particular are focused primarily on planetary transits, and eclipsing binaries with eclipse geometries that are parameterised with a few variables, while more complex light curves caused by substructure within the transiting object require customized analysis code. Aims. We present Beyond Circular Eclipsers (BeyonCE), which reduces the parameter space encompassed by the transit of circum-secondary disc (CSD) systems with azimuthally symmetric non-uniform optical depth profiles. By rejecting disc geometries that cannot reproduce the measured gradients within their light curves, we can constrain the size and orientation of discs with complex sub-structure. Methods. We map out all the possible geometries of a disc, calculate the gradients for rings crossing the star, then reject those configurations where the measured gradient of the light curve is greater than the theoretical gradient from the given disc orientation. Results. We present the fitting code BeyonCE and demonstrate its effectiveness in considerably reducing the parameter space of discs that contain azimuthally symmetric structure by analyzing the light curves seen towards J1407 and PDS 110 which are attributed to CSD transits.
ISSN:2331-8422
DOI:10.48550/arxiv.2404.07378