Confirming & detecting circumbinary planets using radial-velocities.
Thanks to its long photometric stares, PLATO will likely identify multiple transiting circumbinary planets. However the duration of its long stares are insufficient to measure circumbinary planet masses accurately using eclipse timing variations of the central binary. In this talk I show our efforts...
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Format: | Conference Object |
Language: | English |
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Zenodo
2021
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Online Access: | https://dx.doi.org/10.5281/zenodo.5557314 https://zenodo.org/record/5557314 |