001     476593
005     20250724151419.0
024 7 _ |a 10.1140/epjc/s10052-022-10034-4
|2 doi
024 7 _ |a Aguilar:2021uzt
|2 INSPIRETeX
024 7 _ |a inspire:1877761
|2 inspire
024 7 _ |a 1434-6044
|2 ISSN
024 7 _ |a 1434-6052
|2 ISSN
024 7 _ |a arXiv:2107.02604
|2 arXiv
024 7 _ |a altmetric:108842264
|2 altmetric
024 7 _ |a WOS:000756842100004
|2 WOS
024 7 _ |a openalex:W3178924494
|2 openalex
037 _ _ |a PUBDB-2022-01805
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2107.02604
|2 arXiv
100 1 _ |a Aguilar, J. A.
|b 0
245 _ _ |a Reconstructing the neutrino energy for in-ice radio detectors: A study for the Radio Neutrino Observatory Greenland (RNO-G)
260 _ _ |a Heidelberg
|c 2022
|b Springer
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1713281440_2951523
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a 23 pages, 20 figures, version accepted at EPJ-C
520 _ _ |a Since 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
536 _ _ |a RadNu - Radio detection of the PeV - EeV cosmic-neutrino flux (805486)
|0 G:(EU-Grant)805486
|c 805486
|f ERC-2018-STG
|x 1
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a neutrino: energy
|2 INSPIRE
650 _ 7 |a showers: energy
|2 INSPIRE
650 _ 7 |a neutrino: interaction
|2 INSPIRE
650 _ 7 |a neutrino: detector
|2 INSPIRE
650 _ 7 |a radio wave
|2 INSPIRE
650 _ 7 |a observatory
|2 INSPIRE
650 _ 7 |a ice
|2 INSPIRE
650 _ 7 |a IceCube
|2 INSPIRE
650 _ 7 |a cascade
|2 INSPIRE
650 _ 7 |a electric field
|2 INSPIRE
650 _ 7 |a quality
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
|e IceCube South Pole Neutrino Observatory
|x 0
700 1 _ |a Allison, P.
|0 P.Allison.1
|b 1
700 1 _ |a Beatty, J. J.
|0 J.J.Beatty.1
|b 2
700 1 _ |a Bernhoff, H.
|0 H.Bernhoff.1
|b 3
700 1 _ |a Besson, D.
|0 P:(DE-H253)PIP1093318
|b 4
700 1 _ |a Bingefors, N.
|0 N.Bingefors.1
|b 5
700 1 _ |a Botner, O.
|0 O.Botner.1
|b 6
700 1 _ |a Bouma, S.
|b 7
700 1 _ |a Buitink, S.
|0 S.Buitink.1
|b 8
700 1 _ |a Carter, K.
|0 K.Carter.2
|b 9
700 1 _ |a Cataldo, M.
|b 10
700 1 _ |a Clark, B. A.
|b 11
700 1 _ |a Curtis-Ginsberg, Z.
|0 C.D.Curtis.1
|b 12
700 1 _ |a Connolly, A.
|0 A.J.Connolly.1
|b 13
700 1 _ |a Dasgupta, P.
|0 P.D.Gupta.1
|b 14
700 1 _ |a de Kockere, S.
|0 Sudipan.De.1
|b 15
700 1 _ |a de Vries, K. D.
|b 16
700 1 _ |a Deaconu, C.
|0 C.Deaconu.1
|b 17
700 1 _ |a DuVernois, M. A.
|0 Michael.A.DuVernois.1
|b 18
700 1 _ |a Glaser, C.
|0 P:(DE-H253)PIP1092123
|b 19
700 1 _ |a Hallgren, A.
|0 A.Hallgren.1
|b 20
700 1 _ |a Hallmann, Steffen
|0 P:(DE-H253)PIP1094260
|b 21
|u desy
700 1 _ |a Hanson, J. C.
|0 J.C.Hanson.2
|b 22
700 1 _ |a Hendricks, B.
|0 B.Hendricks.2
|b 23
700 1 _ |a Hokanson-Fasig, B.
|0 B.HokansonFasig.5
|b 24
700 1 _ |a Hornhuber, C.
|0 C.Hornhuber.1
|b 25
700 1 _ |a Hughes, K.
|0 K.J.Hughes.1
|b 26
700 1 _ |a Karle, A.
|b 27
700 1 _ |a Kelley, J. L.
|b 28
700 1 _ |a Klein, S. R.
|b 29
700 1 _ |a Krebs, R.
|b 30
700 1 _ |a Lahmann, R.
|b 31
700 1 _ |a Latif, U.
|0 U.Latif.2
|b 32
700 1 _ |a Magnuson, M.
|b 33
700 1 _ |a Meures, T.
|b 34
700 1 _ |a Meyers, Zachary Samuel
|0 P:(DE-H253)PIP1091135
|b 35
|u desy
700 1 _ |a Mulrey, K.
|0 K.Mulrey.1
|b 36
700 1 _ |a Nelles, A.
|0 P:(DE-H253)PIP1083021
|b 37
700 1 _ |a Novikov, A.
|b 38
700 1 _ |a Oberla, E.
|0 E.Oberla.1
|b 39
700 1 _ |a Oeyen, B.
|b 40
700 1 _ |a Pandya, H.
|0 H.Pandya.1
|b 41
700 1 _ |a Plaisier, Ilse
|0 P:(DE-H253)PIP1085465
|b 42
700 1 _ |a Pyras, Lilly
|0 P:(DE-H253)PIP1091084
|b 43
|u desy
700 1 _ |a Ryckbosch, D.
|b 44
700 1 _ |a Scholten, O.
|b 45
700 1 _ |a Seckel, D.
|0 D.Seckel.1
|b 46
700 1 _ |a Smith, D.
|b 47
700 1 _ |a Southall, D.
|0 D.Southall.1
|b 48
700 1 _ |a Torres, J.
|b 49
700 1 _ |a Toscano, S.
|0 S.Toscano.1
|b 50
700 1 _ |a Tosi, D.
|0 P:(DE-H253)PIP1005598
|b 51
700 1 _ |a Broeck, D. J. Van Den
|0 C.Van.Den.Broeck.1
|b 52
700 1 _ |a van Eijndhoven, N.
|0 N.van.Eijndhoven.1
|b 53
700 1 _ |a Vieregg, A. G.
|0 Abigail.Goodhue.Vieregg.1
|b 54
700 1 _ |a Welling, Christoph
|0 P:(DE-H253)PIP1085464
|b 55
|e Corresponding author
700 1 _ |a Wissel, S.
|b 56
700 1 _ |a Young, R.
|b 57
700 1 _ |a Zink, A.
|b 58
773 _ _ |a 10.1140/epjc/s10052-022-10034-4
|g Vol. 82, no. 2, p. 147
|0 PERI:(DE-600)1459069-4
|n 2
|p 147
|t The European physical journal / C
|v 82
|y 2022
|x 1434-6044
856 4 _ |u https://bib-pubdb1.desy.de/record/476593/files/EPJC82%282022%29147.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/476593/files/EPJC82%282022%29147.pdf?subformat=pdfa
|x pdfa
|y Restricted
909 C O |o oai:bib-pubdb1.desy.de:476593
|p openaire
|p VDB
|p OpenAPC
|p ec_fundedresources
|p openCost
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 4
|6 P:(DE-H253)PIP1093318
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 19
|6 P:(DE-H253)PIP1092123
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 21
|6 P:(DE-H253)PIP1094260
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 21
|6 P:(DE-H253)PIP1094260
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 35
|6 P:(DE-H253)PIP1091135
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 35
|6 P:(DE-H253)PIP1091135
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 37
|6 P:(DE-H253)PIP1083021
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 37
|6 P:(DE-H253)PIP1083021
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 42
|6 P:(DE-H253)PIP1085465
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 43
|6 P:(DE-H253)PIP1091084
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 51
|6 P:(DE-H253)PIP1005598
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 55
|6 P:(DE-H253)PIP1085464
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
914 1 _ |y 2022
915 p c |a APC keys set
|0 PC:(DE-HGF)0000
|2 APC
915 p c |a Local Funding
|0 PC:(DE-HGF)0001
|2 APC
915 p c |a DFG OA Publikationskosten
|0 PC:(DE-HGF)0002
|2 APC
915 p c |a DOAJ Journal
|0 PC:(DE-HGF)0003
|2 APC
915 _ _ |a Nationallizenz
|0 StatID:(DE-HGF)0420
|2 StatID
|d 2021-01-27
|w ger
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0571
|2 StatID
|b SCOAP3 sponsored Journal
|d 2021-01-27
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b EUR PHYS J C : 2019
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0300
|2 StatID
|b Medline
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0501
|2 StatID
|b DOAJ Seal
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0500
|2 StatID
|b DOAJ
|d 2021-01-27
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b DOAJ : Blind peer review
|d 2021-01-27
915 _ _ |a Creative Commons Attribution CC BY (No Version)
|0 LIC:(DE-HGF)CCBYNV
|2 V:(DE-HGF)
|b DOAJ
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0600
|2 StatID
|b Ebsco Academic Search
|d 2021-01-27
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b ASC
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2021-01-27
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2021-01-27
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2021-01-27
915 _ _ |a IF < 5
|0 StatID:(DE-HGF)9900
|2 StatID
|d 2021-01-27
915 _ _ |a SCOAP3
|0 StatID:(DE-HGF)0570
|2 StatID
920 1 _ |0 I:(DE-H253)Z_ICE-20210408
|k Z_ICE
|l IceCube+NG
|x 0
920 1 _ |0 I:(DE-H253)Z-RAD-20210408
|k Z-RAD
|l RADIO
|x 1
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)Z_ICE-20210408
980 _ _ |a I:(DE-H253)Z-RAD-20210408
980 _ _ |a APC
980 _ _ |a UNRESTRICTED
980 1 _ |a APC


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21