000476593 001__ 476593
000476593 005__ 20250724151419.0
000476593 0247_ $$2doi$$a10.1140/epjc/s10052-022-10034-4
000476593 0247_ $$2INSPIRETeX$$aAguilar:2021uzt
000476593 0247_ $$2inspire$$ainspire:1877761
000476593 0247_ $$2ISSN$$a1434-6044
000476593 0247_ $$2ISSN$$a1434-6052
000476593 0247_ $$2arXiv$$aarXiv:2107.02604
000476593 0247_ $$2altmetric$$aaltmetric:108842264
000476593 0247_ $$2WOS$$aWOS:000756842100004
000476593 0247_ $$2openalex$$aopenalex:W3178924494
000476593 037__ $$aPUBDB-2022-01805
000476593 041__ $$aEnglish
000476593 082__ $$a530
000476593 088__ $$2arXiv$$aarXiv:2107.02604
000476593 1001_ $$aAguilar, J. A.$$b0
000476593 245__ $$aReconstructing the neutrino energy for in-ice radio detectors: A study for the Radio Neutrino Observatory Greenland (RNO-G)
000476593 260__ $$aHeidelberg$$bSpringer$$c2022
000476593 3367_ $$2DRIVER$$aarticle
000476593 3367_ $$2DataCite$$aOutput Types/Journal article
000476593 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1713281440_2951523
000476593 3367_ $$2BibTeX$$aARTICLE
000476593 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000476593 3367_ $$00$$2EndNote$$aJournal Article
000476593 500__ $$a23 pages, 20 figures, version accepted at EPJ-C
000476593 520__ $$aSince summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) is searching for astrophysical neutrinos at energies ${>10}$ PeV by detecting the radio emission from particle showers in the ice around Summit Station, Greenland. We present an extensive simulation study that shows how RNO-G will be able to measure the energy of such particle cascades, which will in turn be used to estimate the energy of the incoming neutrino that caused them. The location of the neutrino interaction is determined using the differences in arrival times between channels and the electric field of the radio signal is reconstructed using a novel approach based on Information Field Theory. Based on these properties, the shower energy can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm of the shower energy after modest quality cuts and estimate how this can constrain the energy of the neutrino. The method presented in this paper is applicable to all similar radio neutrino detectors, such as the proposed radio array of IceCube-Gen2.
000476593 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000476593 536__ $$0G:(EU-Grant)805486$$aRadNu - Radio detection of the PeV - EeV cosmic-neutrino flux (805486)$$c805486$$fERC-2018-STG$$x1
000476593 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
000476593 650_7 $$2INSPIRE$$aneutrino: energy
000476593 650_7 $$2INSPIRE$$ashowers: energy
000476593 650_7 $$2INSPIRE$$aneutrino: interaction
000476593 650_7 $$2INSPIRE$$aneutrino: detector
000476593 650_7 $$2INSPIRE$$aradio wave
000476593 650_7 $$2INSPIRE$$aobservatory
000476593 650_7 $$2INSPIRE$$aice
000476593 650_7 $$2INSPIRE$$aIceCube
000476593 650_7 $$2INSPIRE$$acascade
000476593 650_7 $$2INSPIRE$$aelectric field
000476593 650_7 $$2INSPIRE$$aquality
000476593 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000476593 7001_ $$0P.Allison.1$$aAllison, P.$$b1
000476593 7001_ $$0J.J.Beatty.1$$aBeatty, J. J.$$b2
000476593 7001_ $$0H.Bernhoff.1$$aBernhoff, H.$$b3
000476593 7001_ $$0P:(DE-H253)PIP1093318$$aBesson, D.$$b4
000476593 7001_ $$0N.Bingefors.1$$aBingefors, N.$$b5
000476593 7001_ $$0O.Botner.1$$aBotner, O.$$b6
000476593 7001_ $$aBouma, S.$$b7
000476593 7001_ $$0S.Buitink.1$$aBuitink, S.$$b8
000476593 7001_ $$0K.Carter.2$$aCarter, K.$$b9
000476593 7001_ $$aCataldo, M.$$b10
000476593 7001_ $$aClark, B. A.$$b11
000476593 7001_ $$0C.D.Curtis.1$$aCurtis-Ginsberg, Z.$$b12
000476593 7001_ $$0A.J.Connolly.1$$aConnolly, A.$$b13
000476593 7001_ $$0P.D.Gupta.1$$aDasgupta, P.$$b14
000476593 7001_ $$0Sudipan.De.1$$ade Kockere, S.$$b15
000476593 7001_ $$ade Vries, K. D.$$b16
000476593 7001_ $$0C.Deaconu.1$$aDeaconu, C.$$b17
000476593 7001_ $$0Michael.A.DuVernois.1$$aDuVernois, M. A.$$b18
000476593 7001_ $$0P:(DE-H253)PIP1092123$$aGlaser, C.$$b19
000476593 7001_ $$0A.Hallgren.1$$aHallgren, A.$$b20
000476593 7001_ $$0P:(DE-H253)PIP1094260$$aHallmann, Steffen$$b21$$udesy
000476593 7001_ $$0J.C.Hanson.2$$aHanson, J. C.$$b22
000476593 7001_ $$0B.Hendricks.2$$aHendricks, B.$$b23
000476593 7001_ $$0B.HokansonFasig.5$$aHokanson-Fasig, B.$$b24
000476593 7001_ $$0C.Hornhuber.1$$aHornhuber, C.$$b25
000476593 7001_ $$0K.J.Hughes.1$$aHughes, K.$$b26
000476593 7001_ $$aKarle, A.$$b27
000476593 7001_ $$aKelley, J. L.$$b28
000476593 7001_ $$aKlein, S. R.$$b29
000476593 7001_ $$aKrebs, R.$$b30
000476593 7001_ $$aLahmann, R.$$b31
000476593 7001_ $$0U.Latif.2$$aLatif, U.$$b32
000476593 7001_ $$aMagnuson, M.$$b33
000476593 7001_ $$aMeures, T.$$b34
000476593 7001_ $$0P:(DE-H253)PIP1091135$$aMeyers, Zachary Samuel$$b35$$udesy
000476593 7001_ $$0K.Mulrey.1$$aMulrey, K.$$b36
000476593 7001_ $$0P:(DE-H253)PIP1083021$$aNelles, A.$$b37
000476593 7001_ $$aNovikov, A.$$b38
000476593 7001_ $$0E.Oberla.1$$aOberla, E.$$b39
000476593 7001_ $$aOeyen, B.$$b40
000476593 7001_ $$0H.Pandya.1$$aPandya, H.$$b41
000476593 7001_ $$0P:(DE-H253)PIP1085465$$aPlaisier, Ilse$$b42
000476593 7001_ $$0P:(DE-H253)PIP1091084$$aPyras, Lilly$$b43$$udesy
000476593 7001_ $$aRyckbosch, D.$$b44
000476593 7001_ $$aScholten, O.$$b45
000476593 7001_ $$0D.Seckel.1$$aSeckel, D.$$b46
000476593 7001_ $$aSmith, D.$$b47
000476593 7001_ $$0D.Southall.1$$aSouthall, D.$$b48
000476593 7001_ $$aTorres, J.$$b49
000476593 7001_ $$0S.Toscano.1$$aToscano, S.$$b50
000476593 7001_ $$0P:(DE-H253)PIP1005598$$aTosi, D.$$b51
000476593 7001_ $$0C.Van.Den.Broeck.1$$aBroeck, D. J. Van Den$$b52
000476593 7001_ $$0N.van.Eijndhoven.1$$avan Eijndhoven, N.$$b53
000476593 7001_ $$0Abigail.Goodhue.Vieregg.1$$aVieregg, A. G.$$b54
000476593 7001_ $$0P:(DE-H253)PIP1085464$$aWelling, Christoph$$b55$$eCorresponding author
000476593 7001_ $$aWissel, S.$$b56
000476593 7001_ $$aYoung, R.$$b57
000476593 7001_ $$aZink, A.$$b58
000476593 773__ $$0PERI:(DE-600)1459069-4$$a10.1140/epjc/s10052-022-10034-4$$gVol. 82, no. 2, p. 147$$n2$$p147$$tThe European physical journal / C$$v82$$x1434-6044$$y2022
000476593 8564_ $$uhttps://bib-pubdb1.desy.de/record/476593/files/EPJC82%282022%29147.pdf$$yRestricted
000476593 8564_ $$uhttps://bib-pubdb1.desy.de/record/476593/files/EPJC82%282022%29147.pdf?subformat=pdfa$$xpdfa$$yRestricted
000476593 8767_ $$92022$$d2023-02-10$$eAPC$$jFlatrate$$lSCOAP3
000476593 909CO $$ooai:bib-pubdb1.desy.de:476593$$popenCost$$pec_fundedresources$$pOpenAPC$$pVDB$$popenaire
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1093318$$aExternal Institute$$b4$$kExtern
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1092123$$aExternal Institute$$b19$$kExtern
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1094260$$aDeutsches Elektronen-Synchrotron$$b21$$kDESY
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1094260$$aExternal Institute$$b21$$kExtern
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1091135$$aDeutsches Elektronen-Synchrotron$$b35$$kDESY
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1091135$$aExternal Institute$$b35$$kExtern
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1083021$$aDeutsches Elektronen-Synchrotron$$b37$$kDESY
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1083021$$aExternal Institute$$b37$$kExtern
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1085465$$aDeutsches Elektronen-Synchrotron$$b42$$kDESY
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1091084$$aDeutsches Elektronen-Synchrotron$$b43$$kDESY
000476593 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1005598$$aExternal Institute$$b51$$kExtern
000476593 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1085464$$aDeutsches Elektronen-Synchrotron$$b55$$kDESY
000476593 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0
000476593 9141_ $$y2022
000476593 915pc $$0PC:(DE-HGF)0000$$2APC$$aAPC keys set
000476593 915pc $$0PC:(DE-HGF)0001$$2APC$$aLocal Funding
000476593 915pc $$0PC:(DE-HGF)0002$$2APC$$aDFG OA Publikationskosten
000476593 915pc $$0PC:(DE-HGF)0003$$2APC$$aDOAJ Journal
000476593 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz$$d2021-01-27$$wger
000476593 915__ $$0StatID:(DE-HGF)0571$$2StatID$$aDBCoverage$$bSCOAP3 sponsored Journal$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bEUR PHYS J C : 2019$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0501$$2StatID$$aDBCoverage$$bDOAJ Seal$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bDOAJ : Blind peer review$$d2021-01-27
000476593 915__ $$0LIC:(DE-HGF)CCBYNV$$2V:(DE-HGF)$$aCreative Commons Attribution CC BY (No Version)$$bDOAJ$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5$$d2021-01-27
000476593 915__ $$0StatID:(DE-HGF)0570$$2StatID$$aSCOAP3
000476593 9201_ $$0I:(DE-H253)Z_ICE-20210408$$kZ_ICE$$lIceCube+NG$$x0
000476593 9201_ $$0I:(DE-H253)Z-RAD-20210408$$kZ-RAD$$lRADIO$$x1
000476593 980__ $$ajournal
000476593 980__ $$aVDB
000476593 980__ $$aI:(DE-H253)Z_ICE-20210408
000476593 980__ $$aI:(DE-H253)Z-RAD-20210408
000476593 980__ $$aAPC
000476593 980__ $$aUNRESTRICTED
000476593 9801_ $$aAPC