Titlebook: Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry; Kento Masuda Book 2018 Springer Nature Singa

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Waqar Zia,Michel Sarkis,Klaus Diepold, modeling of the Rossiter-McLaughlin (RM) effect in the radial velocity (RV) times series. While the RM effect is difficult to observe for planets with smaller radii or on wider orbits than hot Jupiters, new methods based on the high-precision photometric data have recently been developed to provid

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Face Localization and Enhancementerence between orbital inclination (almost .) and stellar inclination ., is used to infer the degree of the spin–orbit misalignment. In this chapter, we develop a methodology for determining true stellar obliquity ., combining the analyses of asteroseismology, transit light curves, and the Rossiter–

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Jacques Berleur,Tanguy Ewbank de Wespinle by applying the gravity-darkening method (Sect. .) to existing data of transiting systems obtained by the . space telescope. The methodology, however, is not fully established, given the discrepancy between this method and the spectroscopic one recently reported for the hot Jupiter system Kepler-

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Springer Series in Vision Researchissues that are important to clarify the role of orbital evolution due to dynamical processes: (i) obliquities of stars hosting long-period transiting planets, (ii) origin of intermediate-period giant planets (warm Jupiters) on eccentric orbits, and (iii) possible difference between single- and mult

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Springer Series in Vision Researchissues that are important to clarify the role of orbital evolution due to dynamical processes: (i) obliquities of stars hosting long-period transiting planets, (ii) origin of intermediate-period giant planets (warm Jupiters) on eccentric orbits, and (iii) possible difference between single- and multi-transiting systems.

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