5574329
doi
10.5281/zenodo.5574329
oai:zenodo.org:5574329
user-plato2021
Mazeh, Tsevi
Tel Aviv University
Zucker, Shay
Tel Aviv University
PLATO-Gaia synergy for studying transiting exoplanets
Panahi, Aviad
Tel Aviv University
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
Gaia
<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>
Zenodo
2021-10-15
info:eu-repo/semantics/lecture
5574328
user-plato2021
1634547234.001371
56575997
md5:25430140311cd408e43e398a79d9fe51
https://zenodo.org/records/5574329/files/PLATO-Gaia synergy.pdf
public
10.5281/zenodo.5574328
isVersionOf
doi