Y. Matsubara 研究室
主宰者:Y. Matsubara
名古屋大学
AI 要約(直近 5 年の研究成果)
要約はまだ生成されていません。
※ AI(Claude)が、公開されている論文要旨から研究の問い・手法・主要な発見を事実情報として抽出・再構成して自動生成しています。誤りを含む可能性があるため、正確性は研究室公式情報でご確認ください。
外部リンク
関連研究室(8 件)
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研究成果(85 件)
- [2025] The Microlensing Event Rate and Optical Depth from MOA-II 9 Yr Survey Toward the Galactic BulgeDOI: https://doi.org/10.3847/1538-4357/ada352
- DOI: https://doi.org/10.1051/0004-6361/202452027
- [2025] A comprehensive analysis of three microlensing planet candidates with the planet/binary degeneracyDOI: https://doi.org/10.1093/mnras/staf1893
- [2025] Observation of Solar Neutron Decay Protons by the International Solar Neutron Detection NetworkDOI: https://doi.org/10.22323/1.501.1339
- DOI: https://doi.org/10.22323/1.501.1344
- DOI: https://doi.org/10.1051/0004-6361/202555200
- DOI: https://doi.org/10.18999/2012890
- DOI: https://doi.org/10.1109/percomworkshops65533.2025.00038
- DOI: https://doi.org/10.1016/j.asr.2025.02.026
- DOI: https://doi.org/10.3847/1538-3881/ae1b8f
続きを表示(残り 75 件)閉じる
- DOI: https://doi.org/10.1051/0004-6361/202554182
- [2025] Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source EventsDOI: https://doi.org/10.3847/1538-3881/adc73e
- DOI: https://doi.org/10.1126/science.adn6088
- DOI: https://doi.org/10.1051/0004-6361/202553811
- [2024] Four microlensing giant planets detected through signals produced by minor-image perturbationsDOI: https://doi.org/10.1051/0004-6361/202450221
- [2024] Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field PlanetsDOI: https://doi.org/10.3847/1538-3881/ad3ba3
- [2024] KMT-2023-BLG-1431Lb: A New q < 10<sup>−4</sup> Microlensing Planet from a Subtle SignatureDOI: https://doi.org/10.1088/1538-3873/ad48b8
- DOI: https://doi.org/10.1051/0004-6361/202349063
- DOI: https://doi.org/10.3847/1538-3881/ad2703
- DOI: https://doi.org/10.1016/j.annonc.2024.10.265
- [2024] Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia PredictionsDOI: https://doi.org/10.3847/1538-4357/ad7bb1
- DOI: https://doi.org/10.1093/eurheartj/ehae666.2225
- DOI: https://doi.org/10.1051/0004-6361/202451416
- DOI: https://doi.org/10.1051/0004-6361/202347951
- DOI: https://doi.org/10.1093/mnras/stae1906
- DOI: https://doi.org/10.1051/0004-6361/202449618
- DOI: https://doi.org/10.3847/1538-3881/ace908
- DOI: https://doi.org/10.3390/universe10010016
- DOI: https://doi.org/10.1093/mnras/stad3672
- DOI: https://doi.org/10.1016/j.jastp.2023.106156
- DOI: https://doi.org/10.1051/0004-6361/202347366
- DOI: https://doi.org/10.21468/scipostphysproc.13.001
- DOI: https://doi.org/10.3847/1538-3881/ace688
- DOI: https://doi.org/10.3847/1538-3881/ace689
- DOI: https://doi.org/10.3847/1538-3881/ace96d
- DOI: https://doi.org/10.22323/1.444.1272
- DOI: https://doi.org/10.22323/1.444.0447
- [2023] Brown dwarf companions in binaries detected in the 2021 season high-cadence microlensing surveysDOI: https://doi.org/10.1051/0004-6361/202347014
- DOI: https://doi.org/10.22323/1.444.1273
- DOI: https://doi.org/10.22323/1.444.1256
- DOI: https://doi.org/10.1051/0004-6361/202346667
- [2023] KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signalDOI: https://doi.org/10.1051/0004-6361/202346596
- DOI: https://doi.org/10.1051/0004-6361/202245455
- DOI: https://doi.org/10.1093/mnras/stad1398
- DOI: https://doi.org/10.3847/1538-3881/acbcc8
- [2023] <i>Kepler K2</i>Campaign 9 – II. First space-based discovery of an exoplanet using microlensingDOI: https://doi.org/10.1093/mnras/stad212
- [2023] A Performance Evaluation of Embedded Multi-core Mixed-criticality System Based on PREEMPT_RT LinuxDOI: https://doi.org/10.2197/ipsjjip.31.78
- DOI: https://doi.org/10.5220/0011722100003464
- DOI: https://doi.org/10.3847/1538-3881/ac9d93
- DOI: https://doi.org/10.1016/j.astropartphys.2022.102780
- DOI: https://doi.org/10.1051/0004-6361/202244186
- DOI: https://doi.org/10.3847/1538-3881/ac82b8
- DOI: https://doi.org/10.3847/1538-3881/ac82b8
- [2022] MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf BoundaryDOI: https://doi.org/10.3847/1538-3881/ac78ed
- DOI: https://doi.org/10.1093/mnras/stac2023
- DOI: https://doi.org/10.3847/2041-8213/ac7442
- DOI: https://doi.org/10.1093/mnras/stac1631
- DOI: https://doi.org/10.1051/0004-6361/202243484
- DOI: https://doi.org/10.3847/1538-4365/ac7441
- DOI: https://doi.org/10.1051/0004-6361/202243744
- DOI: https://doi.org/10.1051/0004-6361/202243490
- DOI: https://doi.org/10.1051/0004-6361/202243550
- DOI: https://doi.org/10.1093/mnras/stac674
- DOI: https://doi.org/10.3847/1538-3881/ac4960
- DOI: https://doi.org/10.22323/1.398.0105
- DOI: https://doi.org/10.3847/1538-3881/ac38ad
- DOI: https://doi.org/10.1051/0004-6361/202142495
- DOI: https://doi.org/10.1109/dasc-picom-cbdcom-cyberscitech52372.2021.00022
- DOI: https://doi.org/10.46720/f2020-ves-017
- [2021] Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial PlanetDOI: https://doi.org/10.3847/1538-3881/ac12d4
- DOI: https://doi.org/10.1051/0004-6361/202141939
- DOI: https://doi.org/10.22323/1.395.0301
- DOI: https://doi.org/10.22323/1.395.0348
- DOI: https://doi.org/10.22323/1.395.0386
- DOI: https://doi.org/10.22323/1.395.1264
- DOI: https://doi.org/10.1093/mnras/stab1787
- DOI: https://doi.org/10.3847/1538-3881/abf930
- DOI: https://doi.org/10.1016/j.nima.2021.165326
- DOI: https://doi.org/10.48550/arxiv.2104.02157
- DOI: https://doi.org/10.1016/j.nima.2021.165019
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