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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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发表于 2025-3-21 17:37:48 | 显示全部楼层 |阅读模式
书目名称Exomoons to Galactic Structure
副标题High Precision Studi
编辑Supachai Awiphan
视频video
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
丛书名称Springer Theses
图书封面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
关键词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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,Besançon 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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