October 6, 2021 Poster Open Access

Rowe, J.F.; Jontof-Hutter, D.; Lissauer, J.

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  <dc:creator>Rowe, J.F.</dc:creator>
  <dc:creator>Jontof-Hutter, D.</dc:creator>
  <dc:creator>Lissauer, J.</dc:creator>
  <dc:date>2021-10-06</dc:date>
  <dc:description>The Plato Mission has the unique capacity to provide long-base observations of thousands of stars and their transiting planets. The current mission plan includes a 2-year stare than includes the Kepler Field.  Plato observations have the potential to improve science return from the Kepler field. Including, the reliability of Kepler planet candidates in the low S/N regime, detection of long-period planets and an overall improvement of exoplanet occurrence rates and transit timing variations and long-term stellar variability and stellar cycles.  The low S/N transit regime includes
potential Earth-sized habitable zone planets around Sun-like stars, which is of high intellectual interest.</dc:description>
  <dc:identifier>https://zenodo.org/record/5553422</dc:identifier>
  <dc:identifier>10.5281/zenodo.5553422</dc:identifier>
  <dc:identifier>oai:zenodo.org:5553422</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.5553421</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:title>An assessment of potential Plato Observing strategies to maximize science return from the Kepler Field.</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
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