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Titlebook: Exomoons to Galactic Structure; High Precision Studi Supachai Awiphan Book 2018 Springer International Publishing AG, part of Springer Natu

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書目名稱Exomoons to Galactic Structure
副標(biāo)題High Precision Studi
編輯Supachai Awiphan
視頻videohttp://file.papertrans.cn/319/318636/318636.mp4
概述Nominated as an outstanding PhD thesis by the University of Manchester, Manchester, UK.Demonstrates a new method of detecting exomoons using transit timing variations and transit duration variation te
叢書名稱Springer Theses
圖書封面Titlebook: Exomoons to Galactic Structure; High Precision Studi Supachai Awiphan Book 2018 Springer International Publishing AG, part of Springer Natu
描述.This book presents three major studies covering exomoon and exoplanet detection and characterisation. Firstly, it reports the observations and analysis of the atmosphere of the hot Neptune GJ3470b, one of the lowest-mass planets with a measured atmosphere, using transmission spectroscopy techniques. The result provided improved measurements of Rayleigh scattering in the atmosphere and the first limits on additional planetary companions in the system. The second part discusses modeling a Kepler-like satellite’s ability of a to detect exomoons by looking for transit timing variations and transit duration variations, demonstrating how exomoons can unambiguously be identified from such data.Lastly, the book examines the development of a state-of-the-art Galactic microlensing simulator, which has been made publicly available. It was used to compare with the largest published sample of microlensing events from the MOA-II survey..
出版日期Book 2018
關(guān)鍵詞Microlensing; Habitable Exomoons; Exomoon and Exoplanet Detection; Neptune GJ3470b; Galactic Microlensin
版次1
doihttps://doi.org/10.1007/978-3-319-90957-8
isbn_softcover978-3-030-08141-6
isbn_ebook978-3-319-90957-8Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing AG, part of Springer Nature 2018
The information of publication is updating

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Transit Timing Variation and Transmission Spectroscopy Analyses of the Hot Neptune GJ3470b,olman et?al., Science 330:51, ., Ford et?al., ApJ 750:113, ., Ford et?al., ApJ 756:185, ., Fabrycky et?al., ApJ 750:114, ., Steffen et?al., MNRAS 421:2342, ., Steffen et?al. ApJ 756:186, ., Steffen et?al. MNRAS 428:1077, ., Mazeh et?al., ApJS 208:16, .).
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,Besan?on Model Simulations of MOA-II,calculate the optical depth, average crossing time and event rate of the microlensing events at the Galactic bulge. In a recent study, the MOA-II survey (Sumi et?al, ApJ 778:150, 2013, Sumi et?al. .) determined these parameters from a study of 474 microlensing events in 2006–2007 observation season.
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Book 2018t duration variations, demonstrating how exomoons can unambiguously be identified from such data.Lastly, the book examines the development of a state-of-the-art Galactic microlensing simulator, which has been made publicly available. It was used to compare with the largest published sample of microlensing events from the MOA-II survey..
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