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Exomoons to galactic structure = hig...
~
Awiphan, Supachai.
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Exomoons to galactic structure = high precision studies with the microlensing and transit methods /
Record Type:
Electronic resources : Monograph/item
Title/Author:
Exomoons to galactic structure/ by Supachai Awiphan.
Reminder of title:
high precision studies with the microlensing and transit methods /
Author:
Awiphan, Supachai.
Published:
Cham :Springer International Publishing : : 2018.,
Description:
xxvi, 187 p. :ill., digital ;24 cm.
[NT 15003449]:
Introduction -- TTV and Transmission Spectroscopy of GJ3470b -- Detectability of Habitable Exomoons -- Microlensing Maps of the Galaxy -- Besan¸Con Model Simulations of MOA-II -- Summary and Future Works.
Contained By:
Springer eBooks
Subject:
Extrasolar planets. -
Online resource:
http://dx.doi.org/10.1007/978-3-319-90957-8
ISBN:
9783319909578
Exomoons to galactic structure = high precision studies with the microlensing and transit methods /
Awiphan, Supachai.
Exomoons to galactic structure
high precision studies with the microlensing and transit methods /[electronic resource] :by Supachai Awiphan. - Cham :Springer International Publishing :2018. - xxvi, 187 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- TTV and Transmission Spectroscopy of GJ3470b -- Detectability of Habitable Exomoons -- Microlensing Maps of the Galaxy -- Besan¸Con Model Simulations of MOA-II -- Summary and Future Works.
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.
ISBN: 9783319909578
Standard No.: 10.1007/978-3-319-90957-8doiSubjects--Topical Terms:
814655
Extrasolar planets.
LC Class. No.: QB820
Dewey Class. No.: 523.24
Exomoons to galactic structure = high precision studies with the microlensing and transit methods /
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Introduction -- TTV and Transmission Spectroscopy of GJ3470b -- Detectability of Habitable Exomoons -- Microlensing Maps of the Galaxy -- Besan¸Con Model Simulations of MOA-II -- Summary and Future Works.
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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.
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Physics and Astronomy (Springer-11651)
based on 0 review(s)
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W9347836
電子資源
11.線上閱覽_V
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EB QB820
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