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010   $a981-10-8453-X
024 7 $a10.1007/978-981-10-8453-9
035   $a(CKB)4100000002892690
035   $a(MiAaPQ)EBC5358142
035   $a(DE-He213)978-981-10-8453-9
035   $a(PPN)225548690
035   $a(EXLCZ)994100000002892690
100   $a20180306d2018      u|         0
101 0 $aeng
135   $aurcnu||||||||
181   $ctxt$2rdacontent
182   $cc$2rdamedia
183   $acr$2rdacarrier
200 10$aExploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry /$fby Kento Masuda
205   $a1st ed. 2018.
210  1$aSingapore :$cSpringer Singapore :$cImprint: Springer,$d2018.
215   $a1 online resource (170 pages)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
311   $a981-10-8452-1 
327   $aDiversity of the Extrasolar Worlds -- Measurements of Stellar Obliquities -- Origin of the Misaligned Hot Jupiters: Nature or Nurture? -- Three-dimensional Stellar Obliquities of HAT-P-7 and Kepler-25 from Joint Analysis of Asteroseismology, Transit Light Curve, and the Rossiter?McLaughlin E?ect -- Spin?Orbit Misalignments of Kepler-13Ab and HAT-P-7b from Gravity-Darkened Transit Light Curves -- Probing the Architecture of Hierarchical Multi-Body Systems: Photometric Characterization of the Triply-Eclipsing Triple-Star System KIC 6543674 -- Summary and Future Prospects.
330   $aThis thesis develops and establishes several methods to determine the detailed geometric architecture of transiting exoplanetary systems (planets orbiting around, and periodically passing in front of, stars other than the sun) using high-precision photometric data collected by the Kepler space telescope. It highlights the measurement of stellar obliquity ? the tilt of the stellar equator with respect to the planetary orbital plane(s) ? and presents methods for more precise obliquity measurements in individual systems of particular interest, as well as for measurements in systems that have been out of reach of previous methods. Such information is useful for investigating the dynamical evolution of the planetary orbit, which is the key to understanding the diverse architecture of exoplanetary systems. The thesis also demonstrates a wide range of unique applications of high-precision photometric data, which expand the capability of future space-based photometry.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aPlanetary science
606   $aAstrophysics
606   $aSpace sciences
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
606   $aPlanetary Sciences$3https://scigraph.springernature.com/ontologies/product-market-codes/P22060
606   $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022
606   $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615  0$aPlanetary science.
615  0$aAstrophysics.
615  0$aSpace sciences.
615 14$aAstronomy, Observations and Techniques.
615 24$aPlanetary Sciences.
615 24$aAstrophysics and Astroparticles.
615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
676   $a530
700   $aMasuda$b Kento$4aut$4http://id.loc.gov/vocabulary/relators/aut$0835670
906   $aBOOK
912   $a9910300532903321
996   $aExploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry$91867854
997   $aUNINA