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000315086 020__ $$a978-3-945931-08-0
000315086 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2016-05/27
000315086 0247_ $$2ISSN$$a1435-8077
000315086 0247_ $$2doi$$a10.3204/DESY-PROC-2016-05/27
000315086 0247_ $$2WOS$$aWOS:00
000315086 0247_ $$2inspire$$ainspire:1501324
000315086 037__ $$aPUBDB-2016-05621
000315086 041__ $$aEnglish
000315086 1001_ $$0P:(DE-H253)PIP1006705$$aTluczykont, Martin$$b0
000315086 1112_ $$0C16-03-17$$2inspire$$aMagellan Workshop$$cHamburg$$d2016-03-17 - 2016-03-18$$wGermany
000315086 245__ $$aConnecting neutrino Astrophysics to Multi-TeV to PeV gamma-ray astronomy with TAIGA
000315086 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2016
000315086 29510 $$aTluczykont, M. "Connecting neutrino Astrophysics to Multi-TeV to PeV gamma-ray astronomy with TAIGA" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
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000315086 520__ $$aRecent evidence for neutrinos in the PeV energy range from IceCube provides additional motivation for the search for the most energetic Galactic accelerators. Gamma-ray astronomy is a sound strategy to reach this goal, providing the energy range beyond 10\,TeV can be covered at a sufficient sensitivity level. The energy spectra of most known gamma-ray emitters only reach up to few 10s of TeV. The HEGRA IACT installation reported evidence for gamma-ray energies from the Crab Nebula as high as 80\,TeV. Uncovering their spectral shape up to few 100s of TeV could answer the question whether some of these objects are cosmic ray Pevatrons, i.e. Galactic PeV accelerators. Extending observations beyond this energy range requires very large effective detector areas, as planned by the TAIGA collaboration.
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