中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV

文献类型:期刊论文

作者Veres, P.61; Acciari, V. A.17,18; Ansoldi, S.16,21; Antonelli, L. A.22; Engels, A. Arbet23; Baack, D.24; Babic, A.25; Banerjee, B.26; de Almeida, U. Barres27; Barrio, J. A.28,29
刊名ASTRONOMY & ASTROPHYSICS
出版日期2020-03-30
卷号635页码:10
ISSN号0004-6361
关键词gamma rays: general methods: observational ISM: supernova remnants
DOI10.1051/0004-6361/201936899
英文摘要Aims. We measure the Crab Nebula gamma-ray spectral energy distribution in the 100 TeV energy domain and test the validity of existing leptonic emission models at these high energies.Methods. We used the novel very large zenith angle observations with the MAGIC telescope system to increase the collection area above 10 TeV. We also developed an auxiliary procedure of monitoring atmospheric transmission in order to assure proper calibration of the accumulated data. This employs recording optical images of the stellar field next to the source position, which provides a better than 10% accuracy for the transmission measurements.Results. We demonstrate that MAGIC very large zenith angle observations yield a collection area larger than a square kilometer. In only 56 h of observations, we detect the gamma-ray emission from the Crab Nebula up to 100 TeV, thus providing the highest energy measurement of this source to date with Imaging Atmospheric Cherenkov Telescopes. Comparing accumulated and archival MAGIC and Fermi/LAT data with some of the existing emission models, we find that none of them provides an accurate description of the 1 GeV to 100 TeV gamma-ray signal.
WOS关键词MAJOR UPGRADE ; GAMMA-RAYS ; PULSAR ; ENERGY ; PERFORMANCE ; TELESCOPES ; SPECTRUM ; SYSTEM
资助项目German BMBF ; MPG ; Italian INFN ; INAF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO[FPA2015-69818-P] ; ERDF under the Spanish MINECO[FPA2012-36668] ; ERDF under the Spanish MINECO[FPA2015-68378-P] ; ERDF under the Spanish MINECO[FPA2015-69210-C6-2-R] ; ERDF under the Spanish MINECO[FPA2015-69210-C6-4-R] ; ERDF under the Spanish MINECO[FPA2015-69210C6-6-R] ; ERDF under the Spanish MINECO[AYA2015-71042-P] ; ERDF under the Spanish MINECO[AYA2016-76012-C3-1-P] ; ERDF under the Spanish MINECO[ESP2015-71662-C2-2-P] ; ERDF under the Spanish MINECO[FPA2017-90566-REDC] ; Indian Department of Atomic Energy ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project[DO1-153/28.08.2018] ; Academy of Finland[320045] ; Spanish Centro de Excelencia "Severo Ochoa"[SEV-2016-0588] ; Spanish Centro de Excelencia "Severo Ochoa"[SEV-2015-0548] ; Unidad de Excelencia "Maria de Maeztu"[MDM-2014-0369] ; Croatian Science Foundation (HrZZ)[IP-2016-06-9782] ; University of Rijeka Project[13.12.1.3.02] ; DFG Collaborative Research Centers[SFB823/C4] ; DFG Collaborative Research Centers[SFB876/C3] ; Polish National Research Centre[UMO-2016/22/M/ST9/00382] ; Brazilian MCTIC ; CNPq ; FAPERJ ; MEXT
WOS研究方向Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:000526206100001
资助机构German BMBF ; German BMBF ; MPG ; MPG ; Italian INFN ; Italian INFN ; INAF ; INAF ; Swiss National Fund SNF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO ; ERDF under the Spanish MINECO ; Indian Department of Atomic Energy ; Indian Department of Atomic Energy ; Japanese JSPS ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Academy of Finland ; Academy of Finland ; Spanish Centro de Excelencia "Severo Ochoa" ; Spanish Centro de Excelencia "Severo Ochoa" ; Unidad de Excelencia "Maria de Maeztu" ; Unidad de Excelencia "Maria de Maeztu" ; Croatian Science Foundation (HrZZ) ; Croatian Science Foundation (HrZZ) ; University of Rijeka Project ; University of Rijeka Project ; DFG Collaborative Research Centers ; DFG Collaborative Research Centers ; Polish National Research Centre ; Polish National Research Centre ; Brazilian MCTIC ; Brazilian MCTIC ; CNPq ; CNPq ; FAPERJ ; FAPERJ ; MEXT ; MEXT ; German BMBF ; German BMBF ; MPG ; MPG ; Italian INFN ; Italian INFN ; INAF ; INAF ; Swiss National Fund SNF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO ; ERDF under the Spanish MINECO ; Indian Department of Atomic Energy ; Indian Department of Atomic Energy ; Japanese JSPS ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Academy of Finland ; Academy of Finland ; Spanish Centro de Excelencia "Severo Ochoa" ; Spanish Centro de Excelencia "Severo Ochoa" ; Unidad de Excelencia "Maria de Maeztu" ; Unidad de Excelencia "Maria de Maeztu" ; Croatian Science Foundation (HrZZ) ; Croatian Science Foundation (HrZZ) ; University of Rijeka Project ; University of Rijeka Project ; DFG Collaborative Research Centers ; DFG Collaborative Research Centers ; Polish National Research Centre ; Polish National Research Centre ; Brazilian MCTIC ; Brazilian MCTIC ; CNPq ; CNPq ; FAPERJ ; FAPERJ ; MEXT ; MEXT ; German BMBF ; German BMBF ; MPG ; MPG ; Italian INFN ; Italian INFN ; INAF ; INAF ; Swiss National Fund SNF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO ; ERDF under the Spanish MINECO ; Indian Department of Atomic Energy ; Indian Department of Atomic Energy ; Japanese JSPS ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Academy of Finland ; Academy of Finland ; Spanish Centro de Excelencia "Severo Ochoa" ; Spanish Centro de Excelencia "Severo Ochoa" ; Unidad de Excelencia "Maria de Maeztu" ; Unidad de Excelencia "Maria de Maeztu" ; Croatian Science Foundation (HrZZ) ; Croatian Science Foundation (HrZZ) ; University of Rijeka Project ; University of Rijeka Project ; DFG Collaborative Research Centers ; DFG Collaborative Research Centers ; Polish National Research Centre ; Polish National Research Centre ; Brazilian MCTIC ; Brazilian MCTIC ; CNPq ; CNPq ; FAPERJ ; FAPERJ ; MEXT ; MEXT ; German BMBF ; German BMBF ; MPG ; MPG ; Italian INFN ; Italian INFN ; INAF ; INAF ; Swiss National Fund SNF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO ; ERDF under the Spanish MINECO ; Indian Department of Atomic Energy ; Indian Department of Atomic Energy ; Japanese JSPS ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Academy of Finland ; Academy of Finland ; Spanish Centro de Excelencia "Severo Ochoa" ; Spanish Centro de Excelencia "Severo Ochoa" ; Unidad de Excelencia "Maria de Maeztu" ; Unidad de Excelencia "Maria de Maeztu" ; Croatian Science Foundation (HrZZ) ; Croatian Science Foundation (HrZZ) ; University of Rijeka Project ; University of Rijeka Project ; DFG Collaborative Research Centers ; DFG Collaborative Research Centers ; Polish National Research Centre ; Polish National Research Centre ; Brazilian MCTIC ; Brazilian MCTIC ; CNPq ; CNPq ; FAPERJ ; FAPERJ ; MEXT ; MEXT
源URL[http://ir.bao.ac.cn/handle/114a11/56156]  
专题中国科学院国家天文台
通讯作者Veres, P.
作者单位1.INAF Astron Observ Naples, Naples, Italy
2.Univ Zaragoza, Dept Fis Teor, Zaragoza, Spain
3.Univ Napoli Federico II, Dipartimento Sci Fis, Naples, Italy
4.Complesso Univ Monte S Angelo, INFN, Sez Napoli, Naples, Italy
5.INAF Osservatorio Astrofis & Sci Spazio, Bologna, Italy
6.Weizmann Inst Sci, Dept Particle Phys & Astrophys, Rehovot, Israel
7.Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast, Antrim, North Ireland
8.Rice Univ, Dept Phys & Astron, Houston, TX USA
9.RAS, SAO, Nizhniy Arkhyz, Russia
10.CSIRO Australia Telescope Natl Facil, Paul Wild Observ, Narrabri, NSW, Australia
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Veres, P.,Acciari, V. A.,Ansoldi, S.,et al. MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV[J]. ASTRONOMY & ASTROPHYSICS,2020,635:10.
APA Veres, P..,Acciari, V. A..,Ansoldi, S..,Antonelli, L. A..,Engels, A. Arbet.,...&Young, D. R..(2020).MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV.ASTRONOMY & ASTROPHYSICS,635,10.
MLA Veres, P.,et al."MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV".ASTRONOMY & ASTROPHYSICS 635(2020):10.

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来源:国家天文台

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