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CHEOPS and NGTS in the Gaia era

Dive into the research by Didier Queloz et al. on the bulk structure and composition of planets, addressing the magnitude problem and diversity of bulk density, enhanced by Kepler statistics. Learn about NGTS' location at Paranal and its performance tested in 2010, with connections to the selected ESA mission for launch in 2017 and the Gaia mission.

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CHEOPS and NGTS in the Gaia era

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  1. CHEOPS and NGTS in the Gaia era Didier Queloz et al. Didier.queloz@unige.ch

  2. Bulk structure and composition

  3. Planetatmosphere

  4. Magnitude problem

  5. Diversity of the bulkdensity

  6. Kepler statistics Howard et al. 2010

  7. www.ngtransits.org Belfast, DLR Berlin, Geneva, Leicester, Warwick, U. Catolica

  8. NGTS location: Paranal (ESO)

  9. Performance design tested in 2010

  10. First Unit test at Geneva 3mmag

  11. http://cheops.unibe.ch/ Selected ESA mission for launch in 2017

  12. Gaia connection

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