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I.5 In the United States: the long way to Kepler
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Registos relacionados: I.5 In the United States: the long way to Kepler
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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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I.4 Across the Atlantic: Canada’s MOST
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I.1 The general framework
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I.3 The CoRoT story
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III.7 Planets orbiting stars more massive than the Sun
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I.2 Seeds take root in Europe
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
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III.4 CoRoT planet host stars
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The CoRoT Legacy Book
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Introduction
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III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
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IV.3 The wealth of stellar variability
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V.3 Present and future space missions for ultra-precision photometry
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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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III.9-2 Tidal evolution of CoRoT massive planets and brown dwarfs and of their host stars
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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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Assunto: photometry
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Assunto: bic Book Industry Communication::P Mathematics & science::PH Physics
Assunto: 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
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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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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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Assunto: space mission
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Assunto: bic Book Industry Communication::P Mathematics & science::PH Physics
Assunto: 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
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: Borucki, W.
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I.5 In the United States: the long way to Kepler
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