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Corrigendum: A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations

dc.contributor.authorBuitink, S.
dc.contributor.authorCorstanje, A.
dc.contributor.authorFalcke, H.
dc.contributor.authorHörandel, J.
dc.contributor.authorHuege, T.
dc.contributor.authorNelles, A.
dc.contributor.authorRachen, J.
dc.contributor.authorRossetto, L.
dc.contributor.authorSchellart, P.
dc.contributor.authorScholten, O.
dc.contributor.authorTer Veen, S.
dc.contributor.authorThoudam, S.
dc.contributor.authorTrinh, T.
dc.contributor.authorAnderson, J.
dc.contributor.authorAsgekar, A.
dc.contributor.authorAvruch, I.
dc.contributor.authorBell, M.
dc.contributor.authorBentum, M.
dc.contributor.authorBernardi, G.
dc.contributor.authorBest, P.
dc.contributor.authorBonafede, A.
dc.contributor.authorBreitling, F.
dc.contributor.authorBroderick, J.
dc.contributor.authorBrouw, W.
dc.contributor.authorBrüggen, M.
dc.contributor.authorButcher, H.
dc.contributor.authorCarbone, D.
dc.contributor.authorCiardi, B.
dc.contributor.authorConway, J.
dc.contributor.authorde Gasperin, F.
dc.contributor.authorde Geus, E.
dc.contributor.authorDeller, A.
dc.contributor.authorDettmar, R.
dc.contributor.authorvan Diepen, G.
dc.contributor.authorDuscha, S.
dc.contributor.authorEislöffel, J.
dc.contributor.authorEngels, D.
dc.contributor.authorEnriquez, J.
dc.contributor.authorFallows, R.
dc.contributor.authorFender, R.
dc.contributor.authorFerrari, C.
dc.contributor.authorFrieswijk, W.
dc.contributor.authorGarrett, M.
dc.contributor.authorGrießmeier, J.
dc.contributor.authorGunst, A.
dc.contributor.authorvan Haarlem, M.
dc.contributor.authorHassall, T.
dc.contributor.authorHeald, G.
dc.contributor.authorHessels, J.
dc.contributor.authorHoeft, M.
dc.contributor.authorHorneffer, A.
dc.contributor.authorIacobelli, M.
dc.contributor.authorIntema, Hubertus
dc.contributor.authorJuette, E.
dc.contributor.authorKarastergiou, A.
dc.contributor.authorKondratiev, V.
dc.contributor.authorKramer, M.
dc.contributor.authorKuniyoshi, M.
dc.contributor.authorKuper, G.
dc.contributor.authorvan Leeuwen, J.
dc.contributor.authorLoose, G.
dc.contributor.authorMaat, P.
dc.contributor.authorMann, G.
dc.contributor.authorMarkoff, S.
dc.contributor.authorMcFadden, R.
dc.contributor.authorMcKay-Bukowski, D.
dc.contributor.authorMcKean, J.
dc.contributor.authorMevius, M.
dc.contributor.authorMulcahy, D.
dc.contributor.authorMunk, H.
dc.contributor.authorNorden, M.
dc.contributor.authorOrru, E.
dc.contributor.authorPaas, H.
dc.contributor.authorPandey-Pommier, M.
dc.contributor.authorPandey, V.
dc.contributor.authorPietka, M.
dc.contributor.authorPizzo, R.
dc.contributor.authorPolatidis, A.
dc.contributor.authorReich, W.
dc.contributor.authorRöttgering, H.
dc.contributor.authorScaife, A.
dc.contributor.authorSchwarz, D.
dc.contributor.authorSerylak, M.
dc.contributor.authorSluman, J.
dc.contributor.authorSmirnov, O.
dc.contributor.authorStappers, B.
dc.contributor.authorSteinmetz, M.
dc.contributor.authorStewart, A.
dc.contributor.authorSwinbank, J.
dc.contributor.authorTagger, M.
dc.contributor.authorTang, Y.
dc.contributor.authorTasse, C.
dc.contributor.authorToribio, M.
dc.contributor.authorVermeulen, R.
dc.contributor.authorVocks, C.
dc.contributor.authorVogt, C.
dc.contributor.authorvan Weeren, R.
dc.contributor.authorWijers, R.
dc.contributor.authorWijnholds, S.
dc.contributor.authorWise, M.
dc.contributor.authorWucknitz, O.
dc.contributor.authorYatawatta, S.
dc.contributor.authorZarka, P.
dc.contributor.authorZensus, J.
dc.date.accessioned2019-02-19T04:14:21Z
dc.date.available2019-02-19T04:14:21Z
dc.date.created2019-02-19T03:58:35Z
dc.date.issued2016
dc.identifier.citationBuitink, S. and Corstanje, A. and Falcke, H. and Hörandel, J. and Huege, T. and Nelles, A. and Rachen, J. et al. 2016. Corrigendum: A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations. Nature. 537 (7621).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/73683
dc.identifier.doi10.1038/nature18936
dc.description.abstract

In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre Auger Observatory, as presented at the International Cosmic Ray Conference 2015 (ref. 1). Figure 1 of this Corrigendum shows measurements of the average value of Xmax for the Low Frequency Array (LOFAR), and earlier experiments using different techniques, now including the data from the Pierre Auger Observatory1, specifically the contribution of A. Porcelli. Our values are in agreement with those of ref. 1 within systematic uncertainties. - Nature 531, 70–73 (2016); doi:10.1038/nature16976
dc.publisherNature Publishing Group
dc.titleCorrigendum: A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations
dc.typeJournal Article
dcterms.source.volume537
dcterms.source.number7621
dcterms.source.issn1476-4687
dcterms.source.titleNature
curtin.accessStatusFulltext not available


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