標(biāo)題: Titlebook: Exomoons to Galactic Structure; High Precision Studi Supachai Awiphan Book 2018 Springer International Publishing AG, part of Springer Natu [打印本頁] 作者: 生長變吼叫 時(shí)間: 2025-3-21 17:37
書目名稱Exomoons to Galactic Structure影響因子(影響力)
書目名稱Exomoons to Galactic Structure影響因子(影響力)學(xué)科排名
書目名稱Exomoons to Galactic Structure網(wǎng)絡(luò)公開度
書目名稱Exomoons to Galactic Structure網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Exomoons to Galactic Structure被引頻次
書目名稱Exomoons to Galactic Structure被引頻次學(xué)科排名
書目名稱Exomoons to Galactic Structure年度引用
書目名稱Exomoons to Galactic Structure年度引用學(xué)科排名
書目名稱Exomoons to Galactic Structure讀者反饋
書目名稱Exomoons to Galactic Structure讀者反饋學(xué)科排名
作者: Hemiparesis 時(shí)間: 2025-3-21 20:30 作者: ABIDE 時(shí)間: 2025-3-22 03:42 作者: 弄污 時(shí)間: 2025-3-22 05:51 作者: FID 時(shí)間: 2025-3-22 09:09 作者: Venules 時(shí)間: 2025-3-22 14:42
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, .).作者: Venules 時(shí)間: 2025-3-22 20:32 作者: 叫喊 時(shí)間: 2025-3-22 22:24 作者: 敵手 時(shí)間: 2025-3-23 01:40
,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.作者: gastritis 時(shí)間: 2025-3-23 08:32
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..作者: excursion 時(shí)間: 2025-3-23 11:22 作者: 星球的光亮度 時(shí)間: 2025-3-23 15:25
Detectability of Habitable Exomoons,n and Han .; Liebig, Wambsganss, A&A 520:A68, Liebig and Wambsganss .), pulsar-timing (Lewis et al., ApJ 685:L153, Lewis et?al. .), Rossiter–McLaughlin effect (Simon et al., MNRAS 406:2038, Simon et?al. .) and scatter-peak (Simon et al., MNRAS 419:164,Simon et?al. .).作者: 冷峻 時(shí)間: 2025-3-23 20:25
2190-5053 transit timing variations and transit duration variation te.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 mea作者: Mortal 時(shí)間: 2025-3-24 01:53
https://doi.org/10.1007/978-3-658-34203-6in of planetary systems. As of February 2018, more than 3,600 planets have been confirmed from ground-based and space-based observation, including some super-Earth planets, planets with masses between 1 and 10 ., which have potential to support life.作者: 畸形 時(shí)間: 2025-3-24 03:38 作者: STANT 時(shí)間: 2025-3-24 07:14 作者: lipoatrophy 時(shí)間: 2025-3-24 14:37 作者: BLAND 時(shí)間: 2025-3-24 16:33 作者: WATER 時(shí)間: 2025-3-24 23:02
https://doi.org/10.1007/978-3-319-90957-8Microlensing; Habitable Exomoons; Exomoon and Exoplanet Detection; Neptune GJ3470b; Galactic Microlensin作者: Tincture 時(shí)間: 2025-3-24 23:38
https://doi.org/10.1007/978-3-658-34203-6of modern astronomy. This is not only because of the potential that living things may exist on them, but also to further our understanding of the origin of planetary systems. As of February 2018, more than 3,600 planets have been confirmed from ground-based and space-based observation, including som作者: 浸軟 時(shí)間: 2025-3-25 07:24 作者: MIRE 時(shí)間: 2025-3-25 08:15
Small Cells: A Critical Assessment822:86, .). The transit method can detect planets ranging in size from Earth to larger than Jupiter. The transit timing variation (TTV) method has been used to find at least 10 additional exoplanets and a hundred of candidates (Agol et al., MNRAS 359:567, ., Holman and Murray, Science 307:1288, ., H作者: 消息靈通 時(shí)間: 2025-3-25 12:44
https://doi.org/10.1007/978-3-642-36508-9 a gas giant, MOA-2011-BLG-262L b (Bennett et?al, ApJ 785:155, .) and a Neptune-sized exomoon orbiting a Jupiter-sized exoplanet, Kepler-1625b I (Teachey et al., (2018) AJ 155:36, .) have been announced. However, if our Solar System is typical, then exomoons must be common. Several methods have been作者: 痛打 時(shí)間: 2025-3-25 17:31
Quantum Devices for Future CSICsalactic bulge (Hamadache et?al. in A & A 454:185, .; Popowski et?al. in ApJ 631:879, .; Sumi et?al. in ApJ 591:204, .; Sumi et?al. in ApJ 636:240, .; Sumi et?al. in ApJ 778:150, .; Wyrzykowski et?al. in ApJS 216:12, .; Mróz et?al. in Nature 548:183, .). The microlensing optical depth, average time s作者: agonist 時(shí)間: 2025-3-25 21:00 作者: consolidate 時(shí)間: 2025-3-26 03:02
https://doi.org/10.1007/978-3-322-82328-1In this thesis, wide-ranging studies on exoplanets and Galactic structure using the microlensing and transit techniques were presented. As the research in these areas is still progressing, there is a lot of things that can be done in the future.作者: Arctic 時(shí)間: 2025-3-26 06:33 作者: 漂白 時(shí)間: 2025-3-26 10:09 作者: 道學(xué)氣 時(shí)間: 2025-3-26 16:02 作者: ligature 時(shí)間: 2025-3-26 17:19 作者: organism 時(shí)間: 2025-3-26 22:26 作者: 休閑 時(shí)間: 2025-3-27 03:23 作者: 過濾 時(shí)間: 2025-3-27 06:29
Detectability of Habitable Exomoons, a gas giant, MOA-2011-BLG-262L b (Bennett et?al, ApJ 785:155, .) and a Neptune-sized exomoon orbiting a Jupiter-sized exoplanet, Kepler-1625b I (Teachey et al., (2018) AJ 155:36, .) have been announced. However, if our Solar System is typical, then exomoons must be common. Several methods have been作者: champaign 時(shí)間: 2025-3-27 10:24 作者: Jargon 時(shí)間: 2025-3-27 17:20 作者: Cupping 時(shí)間: 2025-3-27 20:53 作者: Intentional 時(shí)間: 2025-3-28 01:09 作者: 體貼 時(shí)間: 2025-3-28 05:47 作者: 用手捏 時(shí)間: 2025-3-28 08:39
Gnathifera,nites Rotifera, Acanthocephala, Seisonida) (Fig. 1.1). With the discovery of . (Kristensen and Funch 2000), the taxon Micrognathozoa has been included into the Gnathifera. The name Gnathifera is based on the presence of a complex jaw apparatus in the pharynx of all groups, except Acanthocephala (S?r
