KMS of Xinjiang Astronomical Observatory, CAS
MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV | |
Veres, P.1; Acciari, V. A.98,99; Ansoldi, S.97,102; Antonelli, L. A.103; Engels, A. Arbet104; Baack, D.105; Babic, A.106; Banerjee, B.107; de Almeida, U. Barres108; Barrio, J. A.109,110; Gonzalez, J. Becerra98,99; Bednarek, W.111; Bellizzi, L.109,110; Bernardini, E.114,115,116; Berti, A.117; Besenrieder, J.118; Bhattacharyya, W.114; Bigongiari, C.103; Biland, A.104; Blanch, O.119; Bonnoli, G.109,110; Bosnjak, Z.106; Busetto, G.115,116; Carosi, R.120,121; Ceribella, G.118; Chai, Y.118; Chilingaryan, A.123; Cikota, S.106; Colak, S. M.119; Colin, U.118; Colombo, E.1; Contreras, J. L.109,110; Cortina, J.123; Covino, S.103; D'Elia, V.103; Da Vela, P.120,121; Dazzi, F.103; De Angelis, A.115,116; De Lotto, B.97; Delfino, M.119,124; Delgado, J.119,124; Depaoli, D.117; Di Pierro, F.117; Di Venere, L.117; Espineira, E. Do Souto125; Prester, D. Dominis123; Donini, A.97; Dorner, D.126; Doro, M.115,116; Elsaesser, D.105; Ramazani, V. 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A.47; Xu, D.97; Yaron, O.67; Young, D. R.67 | |
2020-03-30 | |
Source Publication | ASTRONOMY & ASTROPHYSICS
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ISSN | 0004-6361 |
Volume | 635Pages:10 |
Abstract | 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. |
Corresponding Author | Veres, P.() |
Keyword | gamma rays: general methods: observational ISM: supernova remnants |
DOI | 10.1051/0004-6361/201936899 |
Indexed By | SCI ; SCI |
Language | 英语 |
WOS Keyword | MAJOR UPGRADE ; GAMMA-RAYS ; PULSAR ; ENERGY ; PERFORMANCE ; TELESCOPES ; SPECTRUM ; SYSTEM |
Funding Project | 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 Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000526206100001 |
Publisher | EDP SCIENCES S A |
Funding Organization | German BMBF ; MPG ; Italian INFN ; INAF ; Swiss National Fund SNF ; ERDF under the Spanish MINECO ; Indian Department of Atomic Energy ; Japanese JSPS ; Bulgarian Ministry of Education and Science, National RI Roadmap Project ; Academy of Finland ; Spanish Centro de Excelencia Severo Ochoa ; Unidad de Excelencia Maria de Maeztu ; Croatian Science Foundation (HrZZ) ; University of Rijeka Project ; DFG Collaborative Research Centers ; Polish National Research Centre ; Brazilian MCTIC ; CNPq ; FAPERJ ; MEXT |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/6444 |
Collection | 中国科学院新疆天文台 |
Corresponding Author | Veres, P. |
Affiliation | 1.Univ Alabama, Ctr Space Plasma & Aeron Res, Huntsville, AL 35899 USA 2.Univ Alabama, Space Sci Dept, Huntsville, AL 35899 USA 3.Univ Space Res Assoc, Sci & Technol Inst, Huntsville, AL USA 4.NASA, Astrophys Branch, ST12, Marshall Space Flight Ctr, Huntsville, AL USA 5.Max Planck Inst Extraterr Phys, Garching, Germany 6.Kanazawa Univ, Inst Sci & Engn, Fac Math & Phys, Kanazawa, Ishikawa, Japan 7.Univ Maryland, Dept Phys, College Pk, MD 20742 USA 8.NASA, Astrophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD USA 9.Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba, Japan 10.Stockholm Univ, Dept Phys, Stockholm, Sweden 11.KTH Royal Inst Technol, Dept Phys, Stockholm, Sweden 12.Ist Nazl Fis Nucl, Trieste, Italy 13.Univ Politecn Bari, Dipartimento Fis M Merlin, Bari, Italy 14.Ist Nazl Fis Nucl, Sez Bari, Bari, Italy 15.Univ Johannesburg, Dept Phys, Auckland Pk, South Africa 16.Open Univ Israel, Dept Nat Sci, Raanana, Israel 17.Kavli Inst Particle Astrophys & Cosmol, Dept 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Laguna, Inst Astrofis Canarias, San Cristobal la Laguna, Spain 99.Univ La Laguna, Dept Astrofis, San Cristobal la Laguna, Spain 100.Univ Udine, Udine, Italy 101.INFN Trieste, Udine, Italy 102.Kyoto Univ, Dept Phys, Japanese MAGIC Consortium, Kyoto, Japan 103.Natl Inst Astrophys INAF, Rome, Italy 104.Swiss Fed Inst Technol, Zurich, Switzerland 105.Tech Univ Dortmund, Dortmund, Germany 106.Univ Zagreb, Croatian Consortium, FER, Zagreb, Croatia 107.HBNI, Saha Inst Nucl Phys, Kolkata, India 108.CBPF, Rio De Janeiro, Brazil 109.Univ Complutense Madrid, IPARCOS Inst, Madrid, Spain 110.Univ Complutense Madrid, EMFTEL Dept, Madrid, Spain 111.Univ Lodz, Dept Astrophys, Lodz, Poland 112.Univ Siena, Siena, Italy 113.INFN Pisa, Siena, Italy 114.Deutsches Elektronen Synchrotron DESY, Zeuthen, Germany 115.Univ Padua, Padua, Italy 116.INFN, Padua, Italy 117.Ist Nazl Fis Nucl, Frascati, Italy 118.Max Planck Inst Phys & Astrophys, Munich, Germany 119.BIST, IFAE, Barcelona, Spain 120.Univ Pisa, Pisa, Italy 121.INFN Pisa, Pisa, Italy 122.A Alikhanyan Natl Lab, Armenian Consortium, Yerevan, Armenia 123.Ctr Invest Energet Medioambientales & Tecnol, Madrid, Spain 124.PIC, Barcelona, Spain 125.Univ Rijeka, Dept Phys, Croatian Consortium, Rijeka, Croatia 126.Univ Wurzburg, Wurzburg, Germany 127.Univ Turku, Finnish Ctr Astron ESO FINCA, Finnish MAGIC Consortium, Turku, Finland 128.Univ Autonoma Barcelona, Dept Fis, Bellaterra, Spain 129.Univ Autonoma Barcelona, CERES IEEC, Bellaterra, Spain 130.Univ Tokyo, ICRR, Japanese MAGIC Consortium, Kashiwa, Chiba, Japan 131.NAS RA, ICRANet Armenia, Armenian Consortium, Yerevan, Armenia 132.Univ Split, Croatian Consortium, FESB, Split, Croatia 133.Josip Juraj Strossmayer Univ Osijek, Croatian Consortium, Osijek, Croatia 134.RIKEN, Japanese MAGIC Consortium, Wako, Saitama, Japan 135.Tokai Univ, Japanese MAGIC Consortium, Hiratsuka, Kanagawa, Japan 136.Univ Trieste, Dipartimento Fis, Trieste, Italy 137.IFPU, Trieste, Italy 138.Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy, Sofia, Bulgaria 139.Univ Barcelona, ICCUB, IEEC UB, Barcelona, Spain 140.Univ Oulu, Astron Res Unit, Finnish MAGIC Consortium, Oulu, Finland 141.Rudjer Boskovic Inst, Croatian Consortium, Zagreb, Croatia |
Recommended Citation GB/T 7714 | 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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