Published November 12, 2022
| Version v1
Poster
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Automating eclipsing binary light curve analysis: From TESS raw light curve to orbital configuration
Authors/Creators
- 1. KU Leuven
- 2. Radboud University Nijmegen
Description
Analysing and modelling thousands of eclipsing binary light curves is a methodologically and computationally challenging endeavour, certainly in the presence of intrinsic variability. With this poster, we present a conceptually new automated method designed to provide realistic estimates of fundamental orbital parameters of eclipsing binary systems, even in the presence of intrinsic stellar variability.
Notes
Poster 7
Files
2022-10-14_ImBaSE.pdf
Files
(6.2 MB)
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