Astronomia UDP

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Modelado combinado de velocidad radial y astrometría para limitar la población de gigantes gaseosos en órbita amplia.

We use precision radial-velocity instruments in Chile to uncover the first Jupiter-analogues orbiting metal-rich stars.  The key to our project is the combination with space-based astrometric measurements taken by Hipparcos and Gaia, whereby we are developing statistical models that can search the parameter space using a joint model to not only detect these planets, but also to measure their absolute masses and orbital characteristics.

Type of project: PhD thesis
Status: Ongoing
Investigadores Pablo Peña & James Jenkins
Funding source: Basal CATA2, CASACA

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