標(biāo)題: Titlebook: Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates; Observation with the Sei Kato Book 2024 The Editor(s) (if app [打印本頁] 作者: formation 時間: 2025-3-21 19:19
書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影響因子(影響力)
書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影響因子(影響力)學(xué)科排名
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書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates網(wǎng)絡(luò)公開度學(xué)科排名
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書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates讀者反饋
書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates讀者反饋學(xué)科排名
作者: 平常 時間: 2025-3-21 23:03
Tibet Air Shower Array and the Muon Detector Array,ray covers a geometrical area of . and captures extensive air showers initiated by primary particles to estimate their incoming directions and energies. The MD array with a geometrical area of . installed underground counts the number of muons contained in air showers and discriminates CR- and gamma作者: 認(rèn)識 時間: 2025-3-22 02:25
Data Analysis,?to . from the conventional range up?to . in previous studies. The extension improves the photon statistics by . for the sources studied in this work. From a Monte Carlo analysis, the angular and energy resolutions of the experiment for sub-PeV gamma rays are estimated to be . and ., respectively. T作者: 人類 時間: 2025-3-22 07:37 作者: GREG 時間: 2025-3-22 10:29 作者: Demulcent 時間: 2025-3-22 16:36
978-981-97-1645-6The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor作者: Demulcent 時間: 2025-3-22 20:57 作者: 來這真柔軟 時間: 2025-3-22 21:15 作者: 表臉 時間: 2025-3-23 03:50
Vertragskosten und Technologie,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.作者: 易于 時間: 2025-3-23 07:27
Conclusions and Future Prospects,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.作者: 散開 時間: 2025-3-23 11:07 作者: 詳細(xì)目錄 時間: 2025-3-23 16:52
https://doi.org/10.1007/978-3-662-55658-0ray covers a geometrical area of . and captures extensive air showers initiated by primary particles to estimate their incoming directions and energies. The MD array with a geometrical area of . installed underground counts the number of muons contained in air showers and discriminates CR- and gamma作者: hermetic 時間: 2025-3-23 18:03
https://doi.org/10.1007/978-3-8349-6973-6?to . from the conventional range up?to . in previous studies. The extension improves the photon statistics by . for the sources studied in this work. From a Monte Carlo analysis, the angular and energy resolutions of the experiment for sub-PeV gamma rays are estimated to be . and ., respectively. T作者: fibroblast 時間: 2025-3-24 00:10 作者: left-ventricle 時間: 2025-3-24 03:04 作者: 步兵 時間: 2025-3-24 07:34
Sei KatoIs nominated as an outstanding Ph.D. thesis by the University of Tokyo, Japan.Provides pioneering studies of the rapidly expanding sub-PeV gamma-ray astronomy.Includes multi-messenger studies suggesti作者: muffler 時間: 2025-3-24 14:43
2190-5053 amma-ray astronomy.Includes multi-messenger studies suggestiThis book presents two candidates for astrophysical accelerators of cosmic rays with petaelectron-volt (PeV) energies in our Galaxy, the so-called PeVatrons, through the observation of sub-PeV gamma rays performed by the Tibet air shower ar作者: 枕墊 時間: 2025-3-24 15:57
Book 2024atrons, through the observation of sub-PeV gamma rays performed by the Tibet air shower array. The two gamma-ray sources are TASG J1844-038—a newly detected source in this presented work—and HESS J1849-000. Reconstructing their gamma-ray energy spectra up to the sub-PeV range and also analyzing the 作者: Fracture 時間: 2025-3-24 21:14
Book 2024amma-ray sources are candidates for PeVatrons. The results give insights into the population of PeVatron in the Galaxy, which is important to consider their contribution to the PeV cosmic rays observed at the Earth..作者: Melanoma 時間: 2025-3-25 03:00 作者: apropos 時間: 2025-3-25 04:29
,Irreversibilit?t und versunkene Kosten, the other hand, other nearby sources, such as a gamma-ray pulsar (PSR) J1844?0346 and a star forming region N49, could also be the origins of the observed gamma-ray emission, and future deep observations in the radio, infrared, and X-ray bands are required to examine our scenario.作者: 悲痛 時間: 2025-3-25 11:29 作者: 營養(yǎng) 時間: 2025-3-25 13:06
Tibet Air Shower Array and the Muon Detector Array,ed probe calibration measures the transit time of the signals in the PMTs installed on the AS detectors. These calibration methods help us to remove instrumental biases included in the recorded data and reduce the systematic uncertainties in the estimation of the physical parameters of air showers and primary particles.作者: Counteract 時間: 2025-3-25 16:11
,Result 1: Detection of?a?New Gamma-Ray Source TASG J1844?038 in?the?HESS J1843?033 Region, the other hand, other nearby sources, such as a gamma-ray pulsar (PSR) J1844?0346 and a star forming region N49, could also be the origins of the observed gamma-ray emission, and future deep observations in the radio, infrared, and X-ray bands are required to examine our scenario.作者: 丑惡 時間: 2025-3-25 21:49 作者: 我邪惡 時間: 2025-3-26 03:01
https://doi.org/10.1007/978-3-658-25573-2 lack of detail studies of the individual sources. This work observes two gamma-ray sources HESS J1843. and HESS J1849?000 in the sub-PeV energy range and discusses the potential PeVatron nature of these sources.作者: 痛苦一下 時間: 2025-3-26 05:44 作者: Chauvinistic 時間: 2025-3-26 09:51
https://doi.org/10.1007/978-3-8349-6973-6c uncertainty in pointing is estimated through the observation of the Crab Nebula; for TASG J1844?038, it is . and . along the right ascension and the declination, respectively, and for HESS J1849?000, . and ..作者: V切開 時間: 2025-3-26 15:29 作者: Lobotomy 時間: 2025-3-26 19:10 作者: 放大 時間: 2025-3-26 23:45
Data Analysis,c uncertainty in pointing is estimated through the observation of the Crab Nebula; for TASG J1844?038, it is . and . along the right ascension and the declination, respectively, and for HESS J1849?000, . and ..作者: 用肘 時間: 2025-3-27 04:00
Conference proceedings 2022h Performance Cloud Computing.Chapter “Compiler-Assisted Instrumentation Selection for Large-Scale C++ Codes” is available open access under a Creative Commons Attribution 4.0 International License via?link.springer.com..作者: left-ventricle 時間: 2025-3-27 08:24
Sebastian Ertingerlora una matematica del destino, qualcosa come il principio di minima azione di Hamilton, che date le condizioni iniziali di un mondo macroscopico determina in maniera univoca lo stato futuro del mondo stesso? Per quanto increduli, la risposta deve essere: sì..978-88-470-2003-0978-88-470-2004-7Series ISSN 2239-7477 Series E-ISSN 2239-7663 作者: IRATE 時間: 2025-3-27 09:57 作者: aristocracy 時間: 2025-3-27 14:15 作者: 認(rèn)識 時間: 2025-3-27 19:42 作者: 掙扎 時間: 2025-3-27 22:33
2190-5053 r sensitivity with respect to existing techniques. In combination with searches in different decay channels, the presented work contributed to the first observations of?.tt?H.?.production and H?→?bb??decays..978-3-030-65382-8978-3-030-65380-4Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 無能的人 時間: 2025-3-28 02:11
