October 15, 2021 Presentation Open Access

Panahi, Aviad; Mazeh, Tsevi; Zucker, Shay

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{
  "inLanguage": {
    "alternateName": "eng", 
    "@type": "Language", 
    "name": "English"
  }, 
  "description": "<p>By the time PLATO launches, Gaia data is assumed to be all public,<br>\nincluding the epoch data of photometry, astrometry and radial velocities<br>\n(RV). These data offer many possibilities for augmenting PLATO findings. The<br>\nhigh angular resolution of Gaia provides separate light curves of stars<br>\nincluded in the wide PSF of PLATO, thus allowing immediate elimination of<br>\nfalse positives by background eclipsing binaries and, in other cases,<br>\nconfirming that the PLATO transits are indeed originating from the target<br>\nstars.&nbsp;A similar synergy between Gaia and TESS is already taking place<br>\nusing non-public Gaia data, some results are given in this presentation.<br>\nFinally, we show the first transiting exoplanet detected by Gaia - Gaia-1 b.</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "Tel Aviv University", 
      "@id": "https://orcid.org/0000-0001-5850-4373", 
      "@type": "Person", 
      "name": "Panahi, Aviad"
    }, 
    {
      "affiliation": "Tel Aviv University", 
      "@id": "https://orcid.org/0000-0002-3569-3391", 
      "@type": "Person", 
      "name": "Mazeh, Tsevi"
    }, 
    {
      "affiliation": "Tel Aviv University", 
      "@id": "https://orcid.org/0000-0003-3173-3138", 
      "@type": "Person", 
      "name": "Zucker, Shay"
    }
  ], 
  "url": "https://zenodo.org/record/5574329", 
  "datePublished": "2021-10-15", 
  "keywords": [
    "Gaia"
  ], 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5574329", 
  "@id": "https://doi.org/10.5281/zenodo.5574329", 
  "@type": "PresentationDigitalDocument", 
  "name": "PLATO-Gaia synergy for studying transiting exoplanets"
}