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III.3 CoRoT’s planets: A family portrait
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Títulos similares: III.3 CoRoT’s planets: A family portrait
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III.4 CoRoT planet host stars
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III.9-1 Investigating star-planet interactions with CoRoT
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I.3 The CoRoT story
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II.1 The CoRoT observations
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The CoRoT Legacy Book
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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.1 Transit features detected by the CoRoT/Exoplanet Science Team
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V.2 CoRoT heritage in future missions
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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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III.5 Stellar classification in CoRoT faint stars fields
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III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
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II.5 Where to find the CoRoT data?
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III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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III.9 Star-planet Interactions
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III.2 Activity modelling and impact on planet’s parameters
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III.7 Planets orbiting stars more massive than the Sun
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V.3 Present and future space missions for ultra-precision photometry
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I.2 Seeds take root in Europe
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IV.3 The wealth of stellar variability
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II.2 Description of processes and corrections from observation to delivery
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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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Topic: photometry
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Topic: thema EDItEUR::P Mathematics and Science::PH Physics
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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
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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
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I.1 The general framework
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Foreword
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I.3 The CoRoT story
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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
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Spectral Line Shapes in Astrophysics and Related Topics
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Topic: space mission
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Topic: thema EDItEUR::P Mathematics and Science::PH Physics
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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
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I.4 Across the Atlantic: Canada’s MOST
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Autor: Guillot, T.
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III.3 CoRoT’s planets: A family portrait
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Autor: Havel, M.
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III.3 CoRoT’s planets: A family portrait
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