標(biāo)題: Titlebook: Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry; Kento Masuda Book 2018 Springer Nature Singa [打印本頁] 作者: Tyler 時間: 2025-3-21 16:07
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書目名稱Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry影響因子(影響力)學(xué)科排名
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書目名稱Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry讀者反饋
書目名稱Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry讀者反饋學(xué)科排名
作者: Narrative 時間: 2025-3-21 21:27 作者: 王得到 時間: 2025-3-22 03:15
Measurements of Stellar Obliquities,e complimentary information on those planets. In this chapter, we review the methods to measure stellar obliquities and summarize our current knowledge from observations. The implications for the formation scenario of hot Jupiters will be discussed in the next chapter.作者: FAWN 時間: 2025-3-22 05:35
2190-5053 analysis of photometric and spectroscopic data.Discusses un.This thesis develops and establishes several methods to determine the detailed geometric architecture of transiting exoplanetary systems (planets orbiting around, and periodically passing in front of, stars other than the sun) using high-p作者: 憤慨一下 時間: 2025-3-22 11:13
Face Localization and Enhancementter and Kepler-25 with two transiting planets and another non-transiting one. We also show that the joint analysis allows for an accurate and precise determination of the numerous parameters characterizing the planetary system, in addition to ..作者: JEER 時間: 2025-3-22 13:39 作者: JEER 時間: 2025-3-22 20:11 作者: 包裹 時間: 2025-3-22 22:09
Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry978-981-10-8453-9Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: Phenothiazines 時間: 2025-3-23 05:00
https://doi.org/10.1007/978-981-10-8453-9Transiting Exoplanet; Formation of Hot Jupiters; Kepler Space Telescope; Stellar Obliquity; The Rossiter作者: 北極人 時間: 2025-3-23 07:16
Kento MasudaNominated as an outstanding Ph.D. thesis by the University of Tokyo Department of Physics.Presents methodology for the self-consistent joint analysis of photometric and spectroscopic data.Discusses un作者: palpitate 時間: 2025-3-23 12:15 作者: 哀求 時間: 2025-3-23 17:35 作者: defendant 時間: 2025-3-23 20:25
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作者: Graphite 時間: 2025-3-24 00:44 作者: 阻塞 時間: 2025-3-24 03:38
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–作者: Blanch 時間: 2025-3-24 07:32
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-作者: 連累 時間: 2025-3-24 11:43 作者: brachial-plexus 時間: 2025-3-24 18:08
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作者: Neonatal 時間: 2025-3-24 19:29
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.作者: Chauvinistic 時間: 2025-3-24 23:41 作者: resilience 時間: 2025-3-25 04:40
2190-5053 s a wide range of unique applications of high-precision photometric data, which expand the capability of future space-based photometry..978-981-13-4155-7978-981-10-8453-9Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: outrage 時間: 2025-3-25 10:22 作者: sebaceous-gland 時間: 2025-3-25 14:03 作者: 難聽的聲音 時間: 2025-3-25 18:16 作者: 拱形大橋 時間: 2025-3-25 21:46
Jacques Berleur,Tanguy Ewbank de Wespin. The results presented in this chapter clarify the validity and limitation of the gravity-darkening method, and also demonstrate the potential of space-based photometry data to characterize exoplanets and their host stars.作者: oxidant 時間: 2025-3-26 00:18
James M. Humber,Robert F. Almeder scenario often involves a hierarchical configuration (see Sect. .), where the orbit of an outer planet/star is much wider than that of the inner planet. For this reason, characterization of hierarchical systems will be a key for the purpose described above. As the first step of such an effort, this作者: Militia 時間: 2025-3-26 07:00
Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry作者: 影響深遠 時間: 2025-3-26 11:20
Diversity of the Extrasolar Worlds,thought we knew about the solar system. One of the goals of exoplanetary science is to understand the diversity in orbital and physical properties in a comprehensive manner. More specifically, we wish to distinguish the features of planetary systems that necessarily result from the law of Nature, fr作者: 犬儒主義者 時間: 2025-3-26 12:52 作者: 項目 時間: 2025-3-26 19:27 作者: 羊齒 時間: 2025-3-26 22:54 作者: trigger 時間: 2025-3-27 02:59 作者: optional 時間: 2025-3-27 08:44 作者: 幼稚 時間: 2025-3-27 13:30 作者: Multiple 時間: 2025-3-27 13:53 作者: 陰險 時間: 2025-3-27 20:17
,Spin–Orbit Misalignments of Kepler-13Ab and HAT-P-7b from Gravity-Darkened Transit Light Curves,le 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-作者: 優(yōu)雅 時間: 2025-3-27 22:28
Probing the Architecture of Hierarchical Multi-Body Systems: Photometric Characterization of the Trgnature of past dynamical interactions. In contrast, the misalignment between planetary orbits in the same system will serve as more direct evidence for the past dynamical event and may also complement the interpretation of obliquity measurements. Indeed, the scenarios for the high-eccentricity migr作者: 熱烈的歡迎 時間: 2025-3-28 02:18
Summary and Future Prospects,issues 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
