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主题: bic Book Industry Communication::P Mathematics & science::PH Physics
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The CoRoT Legacy Book
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Foreword
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Introduction
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I.1 The general framework
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I.2 Seeds take root in Europe
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I.3 The CoRoT story
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I.4 Across the Atlantic: Canada’s MOST
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I.5 In the United States: the long way to Kepler
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Introduction
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II.1 The CoRoT observations
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II.2 Description of processes and corrections from observation to delivery
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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II.4 The “ready to use” CoRoT data
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II.5 Where to find the CoRoT data?
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Introduction
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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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.4 CoRoT planet host stars
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III.5 Stellar classification in CoRoT faint stars fields
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III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
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III.7 Planets orbiting stars more massive than the Sun
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III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
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III.9 Star-planet Interactions
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主题: thema EDItEUR::P Mathematics and Science::PH Physics
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主题: bic Book Industry Communication::P Mathematics & science::PH Physics
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Quick Look
The CoRoT Legacy Book
Quick Look
Foreword
Quick Look
Introduction
Quick Look
I.1 The general framework
Quick Look
I.2 Seeds take root in Europe
Quick Look
I.3 The CoRoT story
Quick Look
I.4 Across the Atlantic: Canada’s MOST
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I.5 In the United States: the long way to Kepler
Quick Look
Introduction
Quick Look
II.1 The CoRoT observations
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II.2 Description of processes and corrections from observation to delivery
Quick Look
II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
Quick Look
II.4 The “ready to use” CoRoT data
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II.5 Where to find the CoRoT data?
Quick Look
Introduction
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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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.4 CoRoT planet host stars
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III.5 Stellar classification in CoRoT faint stars fields
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III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
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III.7 Planets orbiting stars more massive than the Sun
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III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
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III.9 Star-planet Interactions
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作者: Baudin, F.
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作者: Baglin, A.
作者: Chaintreuil, S.
作者: Fridlund, M.
作者: Csizmadia, Sz
作者: Deeg, H.
作者: Deru, A.
作者: Ferraz-Mello, S.
作者: Ferrigno, A.
作者: Gandolfi, D.
作者: Grotsch-Noels, A.
作者: Guterman, P.
作者: Lam-Trong, T.
作者: Lanza, A. F.
作者: Moutou, C.
作者: Ollivier, M.
作者: Samadi, R.
作者: Vandermarcq, O.
作者: Aigrain, S.
作者: Alencar, S. H. P.
作者: Almenara, J.-M.
作者: Auvergne, M.
作者: Ballans, H.
作者: Barros, S.
作者: Barros, S. C. C.
作者: Belkacem, K.
作者: Bellucci, A.
作者: Bordé, P.
作者: Borucki, W.
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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.5 Where to find the CoRoT data?
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III.5 Stellar classification in CoRoT faint stars fields
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IV.3 The wealth of stellar variability
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作者: Deleuil, M.
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作者: Baglin, A.
作者: Chaintreuil, S.
作者: Fridlund, M.
作者: Csizmadia, Sz
作者: Deeg, H.
作者: Deru, A.
作者: Ferraz-Mello, S.
作者: Ferrigno, A.
作者: Gandolfi, D.
作者: Grotsch-Noels, A.
作者: Guterman, P.
作者: Lam-Trong, T.
作者: Lanza, A. F.
作者: Moutou, C.
作者: Ollivier, M.
作者: Samadi, R.
作者: Vandermarcq, O.
作者: Aigrain, S.
作者: Alencar, S. H. P.
作者: Almenara, J.-M.
作者: Auvergne, M.
作者: Ballans, H.
作者: Barros, S.
作者: Barros, S. C. C.
作者: Belkacem, K.
作者: Bellucci, A.
作者: Bordé, P.
作者: Borucki, W.
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Introduction
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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III.2 Activity modelling and impact on planet’s parameters
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III.4 CoRoT planet host stars
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III.5 Stellar classification in CoRoT faint stars fields
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相似书籍: The CoRoT Legacy Book
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Toggle additional channel list for 相似书籍: The CoRoT Legacy Book
相似书籍: Introduction
相似书籍: I.1 The general framework
相似书籍: I.2 Seeds take root in Europe
相似书籍: I.3 The CoRoT story
相似书籍: I.4 Across the Atlantic: Canada’s MOST
相似书籍: I.5 In the United States: the long way to Kepler
相似书籍: Introduction
相似书籍: II.1 The CoRoT observations
相似书籍: II.2 Description of processes and corrections from observation to delivery
相似书籍: II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
相似书籍: II.4 The “ready to use” CoRoT data
相似书籍: II.5 Where to find the CoRoT data?
相似书籍: Introduction
相似书籍: III.1 Transit features detected by the CoRoT/Exoplanet Science Team
相似书籍: III.2 Activity modelling and impact on planet’s parameters
相似书籍: III.3 CoRoT’s planets: A family portrait
相似书籍: III.4 CoRoT planet host stars
相似书籍: III.5 Stellar classification in CoRoT faint stars fields
相似书籍: III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
相似书籍: III.7 Planets orbiting stars more massive than the Sun
相似书籍: III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
相似书籍: III.9 Star-planet Interactions
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III.4 CoRoT planet host stars
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II.5 Where to find the CoRoT data?
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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
Quick Look
II.1 The CoRoT observations
Quick Look
I.3 The CoRoT story
Quick Look
II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
Quick Look
III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
Quick Look
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.3 CoRoT’s planets: A family portrait
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III.9-1 Investigating star-planet interactions with CoRoT
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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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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I.4 Across the Atlantic: Canada’s MOST
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I.5 In the United States: the long way to Kepler
Quick Look
Introduction
Quick Look
IV.3 The wealth of stellar variability
Quick Look
III.7 Planets orbiting stars more massive than the Sun
Quick Look
Introduction
Quick Look
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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相似书籍: Foreword
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相似书籍: Introduction
相似书籍: I.1 The general framework
相似书籍: I.2 Seeds take root in Europe
相似书籍: I.3 The CoRoT story
相似书籍: I.4 Across the Atlantic: Canada’s MOST
相似书籍: I.5 In the United States: the long way to Kepler
相似书籍: Introduction
相似书籍: II.1 The CoRoT observations
相似书籍: II.2 Description of processes and corrections from observation to delivery
相似书籍: II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
相似书籍: II.4 The “ready to use” CoRoT data
相似书籍: II.5 Where to find the CoRoT data?
相似书籍: Introduction
相似书籍: III.1 Transit features detected by the CoRoT/Exoplanet Science Team
相似书籍: III.2 Activity modelling and impact on planet’s parameters
相似书籍: III.3 CoRoT’s planets: A family portrait
相似书籍: III.4 CoRoT planet host stars
相似书籍: III.5 Stellar classification in CoRoT faint stars fields
相似书籍: III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
相似书籍: III.7 Planets orbiting stars more massive than the Sun
相似书籍: III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
相似书籍: III.9 Star-planet Interactions
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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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
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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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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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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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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
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
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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