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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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Títulos similares: II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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The CoRoT Legacy Book
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II.1 The CoRoT observations
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I.3 The CoRoT story
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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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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.5 Stellar classification in CoRoT faint stars fields
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III.9-1 Investigating star-planet interactions with CoRoT
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III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future
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III.1 Transit features detected by the CoRoT/Exoplanet Science Team
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III.6 Exploration of the brown dwarf regime around solar-like stars by CoRoT
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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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II.2 Description of processes and corrections from observation to delivery
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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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IV.3 The wealth of stellar variability
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III.7 Planets orbiting stars more massive than the Sun
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Farbmessung an LED-Systemen
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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: bic Book Industry Communication::P Mathematics & science::PH Physics
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
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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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Topic: space mission
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Topic: bic Book Industry Communication::P Mathematics & science::PH Physics
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
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
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Autor: Guterman, P.
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Autor: Faigler, S.
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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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Autor: Mazeh, T.
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Autor: Faigler, S.
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II.3 Exposure based algorithm for removing systematics out of the CoRoT light curves
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