000600034 001__ 600034
000600034 005__ 20240117214830.0
000600034 0247_ $$2doi$$a10.22323/1.424.0008
000600034 0247_ $$2INSPIRETeX$$aPlaisier:2023lrs
000600034 0247_ $$2inspire$$ainspire:2716531
000600034 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-07696
000600034 037__ $$aPUBDB-2023-07696
000600034 041__ $$aEnglish
000600034 082__ $$a530
000600034 1001_ $$0P:(DE-H253)PIP1085465$$aPlaisier, Ilse$$b0$$eCorresponding author
000600034 1112_ $$a9th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities$$cSantiago de Compostela$$wSpain
000600034 245__ $$aAngular Resolution for the Radio Neutrino Observatory Greenland (RNO-G)
000600034 260__ $$aTrieste$$bSISSA$$c2023
000600034 3367_ $$2DRIVER$$aarticle
000600034 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$mcontrib
000600034 3367_ $$2DataCite$$aOutput Types/Journal article
000600034 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1705499344_1047649
000600034 3367_ $$2BibTeX$$aARTICLE
000600034 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000600034 3367_ $$00$$2EndNote$$aJournal Article
000600034 4900_ $$2Author$$a2716531
000600034 520__ $$aIn the ultra-high energy regime, the low predicted neutrino fluxes are out of reach for currently running neutrino detectors. Larger instrumented volumes are needed to probe these low fluxes. The Radio Neutrino Observatory Greenland (RNO-G) detects in-ice radio waves emitted by neutrino induced particle showers in the Greenlandic ice sheet. Radio waves have a large attenuation length in ice $\mathcal{O}$(1 km) and therefore RNO-G implements a sparse instrumentation to cover an unprecedented volume. The first seven RNO-G stations have been deployed in the summer of 2021 and 2022 and deployment will be ongoing in the next years.This contribution discusses the angular resolution of RNO-G. We use a method that uses a parametrization for the emitted electric field which is forward folded through the detector and matched with the voltage traces as obtained in the antennas of an RNO-G station. We obtain a $\sigma_{68\%}$ angular resolution of 8$^\circ$ for an optimized event set (75$\%$), and $\sigma_{68\%}$=3$^\circ$ for the subset of events which have significant signal strength in two antennas measuring perpendicular electric-field components, such that a good measurement of the polarization can be obtained.
000600034 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000600034 588__ $$aDataset connected to CrossRef Conference, INSPIRE
000600034 650_7 $$2INSPIRE$$aattenuation: length
000600034 650_7 $$2INSPIRE$$aradio wave: emission
000600034 650_7 $$2INSPIRE$$aneutrino: detector
000600034 650_7 $$2INSPIRE$$aangular resolution
000600034 650_7 $$2INSPIRE$$aobservatory
000600034 650_7 $$2INSPIRE$$aice
000600034 650_7 $$2INSPIRE$$aelectric field
000600034 650_7 $$2INSPIRE$$aparametrization
000600034 650_7 $$2INSPIRE$$apolarization
000600034 650_7 $$2INSPIRE$$aUHE
000600034 650_7 $$2INSPIRE$$ashowers
000600034 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000600034 693__ $$0EXP:(DE-H253)RNO-G-20230101$$5EXP:(DE-H253)RNO-G-20230101$$eThe Radio Neutrino Observatory in Greenland$$x1
000600034 7001_ $$0P:(DE-HGF)0$$aRNO-G Collaboration$$b1$$eCollaboration author
000600034 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.424.0008$$p008$$tProceedings of Science / International School for Advanced Studies$$v(ARENA2022)$$x1824-8039$$y2023
000600034 8564_ $$uhttps://bib-pubdb1.desy.de/record/600034/files/ARENA2022_008.pdf$$yOpenAccess
000600034 8564_ $$uhttps://bib-pubdb1.desy.de/record/600034/files/ARENA2022_008.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000600034 909CO $$ooai:bib-pubdb1.desy.de:600034$$popenaire$$popen_access$$pVDB$$pdriver$$pdnbdelivery
000600034 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1085465$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000600034 9131_ $$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$$x0
000600034 9141_ $$y2023
000600034 915__ $$0LIC:(DE-HGF)CCBYNCND4$$2HGFVOC$$aCreative Commons Attribution-NonCommercial-NoDerivs CC BY-NC-ND 4.0
000600034 915__ $$0StatID:(DE-HGF)0501$$2StatID$$aDBCoverage$$bDOAJ Seal$$d2021-04-20T14:42:38Z
000600034 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ$$d2021-04-20T14:42:38Z
000600034 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000600034 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bDOAJ : Editorial review$$d2021-04-20T14:42:38Z
000600034 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2023-08-30
000600034 9201_ $$0I:(DE-H253)Z_ICE-20210408$$kZ_ICE$$lIceCube+NG$$x0
000600034 9201_ $$0I:(DE-H253)Z-RAD-20210408$$kZ-RAD$$lRADIO$$x1
000600034 980__ $$ajournal
000600034 980__ $$aVDB
000600034 980__ $$aUNRESTRICTED
000600034 980__ $$acontrib
000600034 980__ $$aI:(DE-H253)Z_ICE-20210408
000600034 980__ $$aI:(DE-H253)Z-RAD-20210408
000600034 9801_ $$aFullTexts