000642291 001__ 642291 000642291 005__ 20260209140249.0 000642291 0247_ $$2doi$$a10.1088/1748-0221/20/11/P11015 000642291 0247_ $$2INSPIRETeX$$aRNO-G:2025gyt 000642291 0247_ $$2inspire$$ainspire:2937869 000642291 0247_ $$2arXiv$$aarXiv:2506.17522 000642291 0247_ $$2datacite_doi$$a10.3204/PUBDB-2025-05462 000642291 0247_ $$2openalex$$aopenalex:W4416427199 000642291 037__ $$aPUBDB-2025-05462 000642291 041__ $$aEnglish 000642291 082__ $$a610 000642291 088__ $$2arXiv$$aarXiv:2506.17522 000642291 1001_ $$aAgarwal, S.$$b0 000642291 245__ $$aRadio emission from airplanes as observed with RNO-G 000642291 260__ $$aLondon$$bInst. of Physics$$c2025 000642291 3367_ $$2DRIVER$$aarticle 000642291 3367_ $$2DataCite$$aOutput Types/Journal article 000642291 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1768212067_2487194 000642291 3367_ $$2BibTeX$$aARTICLE 000642291 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000642291 3367_ $$00$$2EndNote$$aJournal Article 000642291 520__ $$aThis paper describes how intentional and unintentional radioemission from airplanes is recorded with the Radio NeutrinoObservatory Greenland (RNO-G). We characterize the receivedsignals and define a procedure to extract a clean set of impulsivesignals. These signals are highly suitable for instrumentcalibration, also for future experiments. A set of signals is usedto probe the timing precision of RNO-G in-situ, which is found tomatch expectations. We also discuss the impact of these signals onthe ability to detect neutrinos with RNO-G. 000642291 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0 000642291 536__ $$0G:(EU-Grant)101115122$$aPRO-RNO-G - Discovering neutrinos of extreme energies with the Radio Neutrino Observatory Greenland (101115122)$$c101115122$$fERC-2023-STG$$x1 000642291 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de 000642291 650_7 $$2autogen$$aData analysis 000642291 650_7 $$2autogen$$aInstrumental noise 000642291 650_7 $$2autogen$$aNeutrino detectors 000642291 693__ $$0EXP:(DE-H253)RNO-G-20230101$$5EXP:(DE-H253)RNO-G-20230101$$eThe Radio Neutrino Observatory in Greenland$$x0 000642291 7001_ $$aAguilar, J. A.$$b1 000642291 7001_ $$00009-0003-2076-6118$$aAlden, N.$$b2 000642291 7001_ $$aAli, S.$$b3 000642291 7001_ $$00000-0001-8141-2653$$aAllison, P.$$b4 000642291 7001_ $$00009-0008-9174-7148$$aBetts, M.$$b5 000642291 7001_ $$aBesson, D.$$b6 000642291 7001_ $$aBishop, A.$$b7 000642291 7001_ $$00000-0001-8588-7306$$aBotner, O.$$b8 000642291 7001_ $$0P:(DE-H253)PIP1096020$$aBouma, S.$$b9 000642291 7001_ $$00000-0002-6177-497X$$aBuitink, S.$$b10 000642291 7001_ $$00009-0005-5306-8564$$aCamphyn, R.$$b11 000642291 7001_ $$00000-0002-5465-147X$$aChan, J.$$b12 000642291 7001_ $$00000-0002-2853-5862$$aChiche, S.$$b13 000642291 7001_ $$aClark, B. A.$$b14 000642291 7001_ $$aColeman, A.$$b15 000642291 7001_ $$00000-0001-5311-3648$$aCouberly, K.$$b16 000642291 7001_ $$00000-0001-6724-012X$$ade Kockere, S.$$b17 000642291 7001_ $$ade Vries, K. 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S.$$b48 000642291 7001_ $$00000-0001-8026-8020$$aMulrey, K.$$b49 000642291 7001_ $$00000-0003-4615-5529$$aMuzio, M.$$b50 000642291 7001_ $$0P:(DE-H253)PIP1083021$$aNelles, Anna$$b51 000642291 7001_ $$aNovikov, A.$$b52 000642291 7001_ $$aNozdrina, A.$$b53 000642291 7001_ $$00000-0001-8344-7999$$aOberla, E.$$b54 000642291 7001_ $$aOeyen, B.$$b55 000642291 7001_ $$00009-0003-3201-0115$$aPunsuebsay, N.$$b56 000642291 7001_ $$aPyras, L.$$b57 000642291 7001_ $$00009-0007-6872-8603$$aRavn, M.$$b58 000642291 7001_ $$00009-0003-1010-5156$$aRifaie, A.$$b59 000642291 7001_ $$aRyckbosch, D.$$b60 000642291 7001_ $$aSchlemper, O.$$b61 000642291 7001_ $$aSchlüter, F.$$b62 000642291 7001_ $$aScholten, O.$$b63 000642291 7001_ $$00009-0009-9085-466X$$aSeckel, D.$$b64 000642291 7001_ $$00000-0002-4464-7354$$aSeikh, M. F. 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