生长变吼叫 发表于 2025-3-21 17:37:48

书目名称Exomoons to Galactic Structure影响因子(影响力)<br>        http://figure.impactfactor.cn/if/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure影响因子(影响力)学科排名<br>        http://figure.impactfactor.cn/ifr/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure网络公开度<br>        http://figure.impactfactor.cn/at/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure网络公开度学科排名<br>        http://figure.impactfactor.cn/atr/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure被引频次<br>        http://figure.impactfactor.cn/tc/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure被引频次学科排名<br>        http://figure.impactfactor.cn/tcr/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure年度引用<br>        http://figure.impactfactor.cn/ii/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure年度引用学科排名<br>        http://figure.impactfactor.cn/iir/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure读者反馈<br>        http://figure.impactfactor.cn/5y/?ISSN=BK0318636<br><br>        <br><br>书目名称Exomoons to Galactic Structure读者反馈学科排名<br>        http://figure.impactfactor.cn/5yr/?ISSN=BK0318636<br><br>        <br><br>

Hemiparesis 发表于 2025-3-21 20:30:54

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ABIDE 发表于 2025-3-22 03:42:04

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弄污 发表于 2025-3-22 05:51:25

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FID 发表于 2025-3-22 09:09:39

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Venules 发表于 2025-3-22 14:42:43

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, .).

Venules 发表于 2025-3-22 20:32:19

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叫喊 发表于 2025-3-22 22:24:31

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敌手 发表于 2025-3-23 01:40:17

,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.

gastritis 发表于 2025-3-23 08:32:14

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