Panahi, Aviad
Mazeh, Tsevi
Zucker, Shay
2021-10-15
<p>By the time PLATO launches, Gaia data is assumed to be all public,<br>
including the epoch data of photometry, astrometry and radial velocities<br>
(RV). These data offer many possibilities for augmenting PLATO findings. The<br>
high angular resolution of Gaia provides separate light curves of stars<br>
included in the wide PSF of PLATO, thus allowing immediate elimination of<br>
false positives by background eclipsing binaries and, in other cases,<br>
confirming that the PLATO transits are indeed originating from the target<br>
stars. A similar synergy between Gaia and TESS is already taking place<br>
using non-public Gaia data, some results are given in this presentation.<br>
Finally, we show the first transiting exoplanet detected by Gaia - Gaia-1 b.</p>
https://doi.org/10.5281/zenodo.5574329
oai:zenodo.org:5574329
eng
Zenodo
https://zenodo.org/communities/plato2021
https://doi.org/10.5281/zenodo.5574328
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
Gaia
PLATO-Gaia synergy for studying transiting exoplanets
info:eu-repo/semantics/lecture