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  • I.2 Seeds take root in Europe
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Títulos similares: I.2 Seeds take root in Europe

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    III.2 Activity modelling and impact on planet’s parameters
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    V.2 CoRoT heritage in future missions
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    II.2 Description of processes and corrections from observation to delivery
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    IV.2 Pulsating red giant stars
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    I.1 The general framework
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    I.3 The CoRoT story
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    III.9-2 Tidal evolution of CoRoT massive planets and brown dwarfs and of their host stars
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    III.4 CoRoT planet host stars
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    I.4 Across the Atlantic: Canada’s MOST
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    III.3 CoRoT’s planets: A family portrait
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    III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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    II.1 The CoRoT observations
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    Introduction
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    IV.1 Insights on the internal structure of stars as provided by seismology
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    III.9 Star-planet Interactions
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    Introduction
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    V.3 Present and future space missions for ultra-precision photometry
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    Foreword
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    Introduction
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    III.9-1 Investigating star-planet interactions with CoRoT
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    II.4 The “ready to use” CoRoT data
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    V.1 Lessons learned from CoRoT
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    Introduction
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    I.5 In the United States: the long way to Kepler

Topic: photometry

  • Topic: thema EDItEUR::P Mathematics and Science::PH Physics
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  • Quick Look
    III.1 Transit features detected by the CoRoT/Exoplanet Science Team
  • Quick Look
    II.1 The CoRoT observations
  • Quick Look
    Introduction
  • Quick Look
    IV.1 Insights on the internal structure of stars as provided by seismology
  • Quick Look
    III.9 Star-planet Interactions
  • Quick Look
    Introduction
  • Quick Look
    I.2 Seeds take root in Europe
  • Quick Look
    III.9-2 Tidal evolution of CoRoT massive planets and brown dwarfs and of their host stars
  • Quick Look
    V.3 Present and future space missions for ultra-precision photometry
  • Quick Look
    Optical Systems for Astronomy
  • Quick Look
    III.2 Activity modelling and impact on planet’s parameters
  • Quick Look
    V.2 CoRoT heritage in future missions
  • Quick Look
    IV.2 Pulsating red giant stars
  • Quick Look
    I.1 The general framework
  • Quick Look
    Foreword
  • Quick Look
    I.3 The CoRoT story
  • Quick Look
    Introduction
  • Quick Look
    III.9-1 Investigating star-planet interactions with CoRoT
  • Quick Look
    II.4 The “ready to use” CoRoT data
  • Quick Look
    V.1 Lessons learned from CoRoT
  • Quick Look
    Introduction
  • Quick Look
    II.2 Description of processes and corrections from observation to delivery
  • Quick Look
    III.3 CoRoT’s planets: A family portrait
  • Quick Look
    Spectral Line Shapes in Astrophysics and Related Topics

Topic: space mission

  • Topic: thema EDItEUR::P Mathematics and Science::PH Physics
  • Show items as search results
  • Explore related channels
  • Quick Look
    III.1 Transit features detected by the CoRoT/Exoplanet Science Team
  • Quick Look
    II.1 The CoRoT observations
  • Quick Look
    Introduction
  • Quick Look
    IV.1 Insights on the internal structure of stars as provided by seismology
  • Quick Look
    III.9 Star-planet Interactions
  • Quick Look
    Introduction
  • Quick Look
    I.2 Seeds take root in Europe
  • Quick Look
    III.9-2 Tidal evolution of CoRoT massive planets and brown dwarfs and of their host stars
  • Quick Look
    V.3 Present and future space missions for ultra-precision photometry
  • Quick Look
    III.2 Activity modelling and impact on planet’s parameters
  • Quick Look
    V.2 CoRoT heritage in future missions
  • Quick Look
    IV.2 Pulsating red giant stars
  • Quick Look
    I.1 The general framework
  • Quick Look
    Foreword
  • Quick Look
    I.3 The CoRoT story
  • Quick Look
    Introduction
  • Quick Look
    III.9-1 Investigating star-planet interactions with CoRoT
  • Quick Look
    II.4 The “ready to use” CoRoT data
  • Quick Look
    V.1 Lessons learned from CoRoT
  • Quick Look
    Introduction
  • Quick Look
    II.2 Description of processes and corrections from observation to delivery
  • Quick Look
    III.3 CoRoT’s planets: A family portrait
  • Quick Look
    III.5 Stellar classification in CoRoT faint stars fields
  • Quick Look
    I.4 Across the Atlantic: Canada’s MOST

Autor: Fridlund, M.

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    I.2 Seeds take root in Europe
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    III.4 CoRoT planet host stars
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    III.7 Planets orbiting stars more massive than the Sun

Autor: Roxburgh, I.

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    I.2 Seeds take root in Europe

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