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II.2 Description of processes and corrections from observation to delivery
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II.4 The “ready to use” CoRoT data
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II.1 The CoRoT observations
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V.2 CoRoT heritage in future missions
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I.1 The general framework
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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II.5 Where to find the CoRoT data?
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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I.3 The CoRoT story
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V.3 Present and future space missions for ultra-precision photometry
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IV.3 The wealth of stellar variability
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III.2 Activity modelling and impact on planet’s parameters
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III.3 CoRoT’s planets: A family portrait
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III.9-1 Investigating star-planet interactions with CoRoT
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I.2 Seeds take root in Europe
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IV.1 Insights on the internal structure of stars as provided by seismology
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IV.2 Pulsating red giant stars
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III.9 Star-planet Interactions
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III.5 Stellar classification in CoRoT faint stars fields
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Introduction
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III.7 Planets orbiting stars more massive than the Sun
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I.4 Across the Atlantic: Canada’s MOST
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Sensorfusion zur Kompensation von Messfehlern bei kamerabasierter Farbverteilungsmessung
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Spectral near field data of LED systems for optical simulations
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III.4 CoRoT planet host stars
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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
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Introduction
Quick Look
IV.1 Insights on the internal structure of stars as provided by seismology
Quick Look
III.9 Star-planet Interactions
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Introduction
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I.2 Seeds take root in Europe
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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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V.3 Present and future space missions for ultra-precision photometry
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Optical Systems for Astronomy
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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
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
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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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II.2 Description of processes and corrections from observation to delivery
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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: 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
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II.2 Description of processes and corrections from observation to delivery
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III.3 CoRoT’s planets: A family portrait
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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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Author: Ollivier, M.
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Author: Chaintreuil, S.
Author: Ferrigno, A.
Author: Baglin, A.
Author: Almenara, J.-M.
Author: Auvergne, M.
Author: Barros, S.
Author: Baudin, F.
Author: Boumier, P.
Author: Chabaud, P.-Y.
Author: Deeg, H.
Author: Guterman, P.
Author: Jorda, L.
Author: Samadi, R.
Author: Tuna, T.
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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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Author: Deru, A.
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Author: Chaintreuil, S.
Author: Ferrigno, A.
Author: Baglin, A.
Author: Almenara, J.-M.
Author: Auvergne, M.
Author: Barros, S.
Author: Baudin, F.
Author: Boumier, P.
Author: Chabaud, P.-Y.
Author: Deeg, H.
Author: Guterman, P.
Author: Jorda, L.
Author: Samadi, R.
Author: Tuna, T.
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II.4 The “ready to use” CoRoT data
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II.2 Description of processes and corrections from observation to delivery
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