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000448234 0247_ $$2arXiv$$aarXiv:2004.09841
000448234 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-03343
000448234 037__ $$aPUBDB-2020-03343
000448234 041__ $$aEnglish
000448234 088__ $$2arXiv$$aarXiv:2004.09841
000448234 1001_ $$aAnker, A.$$b0
000448234 245__ $$aWhite Paper: ARIANNA-200 high energy neutrino telescope
000448234 260__ $$c2020
000448234 300__ $$a12
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000448234 520__ $$aThe proposed ARIANNA-200 neutrino detector, located at sea-level on the Ross Ice Shelf, Antarctica, consists of 200 autonomous and independent detector stations separated by 1 kilometer in a uniform triangular mesh, and serves as a pathfinder mission for the future IceCube-Gen2 project. The primary science mission of ARIANNA-200 is to search for sources of neutrinos with energies greater than 10^17 eV, complementing the reach of IceCube. An ARIANNA observation of a neutrino source would provide strong insight into the enigmatic sources of cosmic rays. ARIANNA observes the radio emission from high energy neutrino interactions in the Antarctic ice. Among radio based concepts under current investigation, ARIANNA-200 would uniquely survey the vast majority of the southern sky at any instant in time, and an important region of the northern sky, by virtue of its location on the surface of the Ross Ice Shelf in Antarctica. The broad sky coverage is specific to the Moore's Bay site, and makes ARIANNA-200 ideally suited to contribute to the multi-messenger thrust by the US National Science Foundation, Windows on the Universe - Multi-Messenger Astrophysics, providing capabilities to observe explosive sources from unknown directions. The ARIANNA architecture is designed to measure the angular direction to within 3 degrees for every neutrino candidate, which too plays an important role in the pursuit of multi-messenger observations of astrophysical sources.
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000448234 536__ $$0G:(EU-Grant)646623$$aNEUCOS - Neutrinos and the origin of the cosmic rays (646623)$$c646623$$fERC-2014-CoG$$x1
000448234 588__ $$aDataset connected to arXivarXiv
000448234 650_7 $$2INSPIRE$$aneutrino: detector
000448234 650_7 $$2INSPIRE$$aneutrino: energy: high
000448234 650_7 $$2INSPIRE$$aneutrino: particle source
000448234 650_7 $$2INSPIRE$$aneutrino: interaction
000448234 650_7 $$2INSPIRE$$aARIANNA
000448234 650_7 $$2INSPIRE$$aBaikal
000448234 650_7 $$2INSPIRE$$acosmic radiation: UHE
000448234 650_7 $$2INSPIRE$$acosmic radiation: acceleration
000448234 650_7 $$2INSPIRE$$aice
000448234 650_7 $$2INSPIRE$$abackground
000448234 650_7 $$2INSPIRE$$amuon
000448234 650_7 $$2INSPIRE$$ashowers: electromagnetic
000448234 650_7 $$2INSPIRE$$asensitivity
000448234 650_7 $$2INSPIRE$$acosmic radiation: energy spectrum
000448234 650_7 $$2INSPIRE$$aKM3NeT
000448234 650_7 $$2INSPIRE$$aAuger
000448234 650_7 $$2INSPIRE$$atriangulation
000448234 650_7 $$2INSPIRE$$aradio wave
000448234 650_7 $$2INSPIRE$$asurface
000448234 650_7 $$2INSPIRE$$aIceCube
000448234 650_7 $$2INSPIRE$$athrust
000448234 650_7 $$2INSPIRE$$asite
000448234 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000448234 7001_ $$aBaldi, P.$$b1
000448234 7001_ $$aBarwick, S. W.$$b2
000448234 7001_ $$aBergman, D.$$b3
000448234 7001_ $$aBernhoff, H.$$b4
000448234 7001_ $$aBesson, D. Z.$$b5
000448234 7001_ $$aBingefors, N.$$b6
000448234 7001_ $$aBotner, O.$$b7
000448234 7001_ $$aChen, P.$$b8
000448234 7001_ $$aChen, Y.$$b9
000448234 7001_ $$0P:(DE-HGF)0$$aGarcía-Fernández, D.$$b10
000448234 7001_ $$aGaswint, G.$$b11
000448234 7001_ $$0P:(DE-HGF)0$$aGlaser, C.$$b12$$eCorresponding author
000448234 7001_ $$aHallgren, A.$$b13
000448234 7001_ $$aHanson, J. C.$$b14
000448234 7001_ $$aHuang, J. J.$$b15
000448234 7001_ $$aKlein, S. R.$$b16
000448234 7001_ $$aKleinfelder, S. A.$$b17
000448234 7001_ $$aKuo, C. -Y.$$b18
000448234 7001_ $$aLahmann, R.$$b19
000448234 7001_ $$aLatif, U.$$b20
000448234 7001_ $$aLiu, T.$$b21
000448234 7001_ $$aLyu, Y.$$b22
000448234 7001_ $$aMcAleer, S.$$b23
000448234 7001_ $$aNam, J.$$b24
000448234 7001_ $$aNovikov, A.$$b25
000448234 7001_ $$0P:(DE-H253)PIP1083021$$aNelles, A.$$b26$$udesy
000448234 7001_ $$aPaul, M. P.$$b27
000448234 7001_ $$aPersichilli, C.$$b28
000448234 7001_ $$0P:(DE-H253)PIP1085465$$aPlaisier, I.$$b29
000448234 7001_ $$aShiao, J. Y.$$b30
000448234 7001_ $$aTatar, J.$$b31
000448234 7001_ $$0P:(DE-HGF)0$$avan Vliet, A.$$b32
000448234 7001_ $$aWang, S. -H.$$b33
000448234 7001_ $$aWang, Y. -H.$$b34
000448234 7001_ $$0P:(DE-H253)PIP1085464$$aWelling, C.$$b35
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