October 8, 2021 Presentation Open Access

Amaury H.M.J.Triaud

DCAT Export

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        <foaf:name>Amaury H.M.J.Triaud</foaf:name>
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    <dct:title>Confirming &amp; detecting circumbinary planets using radial-velocities.</dct:title>
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    <dcat:keyword>Exoplanets</dcat:keyword>
    <dcat:keyword>Circumbinary exoplanets</dcat:keyword>
    <dcat:keyword>Binary stars</dcat:keyword>
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    <dcat:keyword>Radial-velocities</dcat:keyword>
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    <dct:description>&lt;p&gt;Thanks to its long photometric stares, PLATO will likely identify multiple&amp;nbsp;transiting circumbinary planets. However the duration of its long stares are&amp;nbsp;insufficient to measure circumbinary planet masses accurately using eclipse&amp;nbsp;timing variations of the central binary. In this talk I show our efforts&amp;nbsp;on HARPS and SOPHIE to detect circumbinary planets orbiting single-lined&amp;nbsp;eclipse binaries. I will show the first ground-based detections of&amp;nbsp;circumbinary planets made by SOPHIE, HARPS in radial-velocities, and the&lt;br&gt; first circumbinary planet transit obtained from ground, using ASTEP in&amp;nbsp;Antarctica. The methods we are developing are key to prepare for the&amp;nbsp;confirmation of PLATO&amp;#39;s circumbinary planets.&lt;br&gt; &lt;br&gt; &amp;nbsp;&lt;/p&gt;</dct:description>
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    <dct:title>Binaries Escorted By Orbiting Planets</dct:title>
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