Publisher’s Note: Indications of Proton-Dominated Cosmic-Ray Composition above 1.6 EeV [phys. Rev. Lett.104, 161101 (2010)]
R. U. Abbasi,T. Abu-Zayyad,M. Al-Seady,M. Allen,J. F. Amman,R. J. Anderson,G. Archbold,K. Belov,J. W. Belz,D. R. Bergman,S. A. Blake,O. A. Brusova,G. W. Burt,C. Cannon,Z. Cao,W. Deng,Y. Fedorova,C. B. Finley,R. C. Gray,W. F. Hanlon,C. M. Hoffman,M. H. Holzscheiter,G. Hughes,P. Hüntemeyer,D. Ivanov,B. F. Jones,C. C. H. Jui, K. Kim,M. A. Kirn,E. C. Loh, J. Liu,J. P. Lundquist,M. M. Maestas,N. Manago,L. J. Marek,K. Martens,J. A. J. Matthews,J. N. Matthews,S. A. Moore,A. O’Neill,C. A. Painter,L. Perera,K. Reil,R. Riehle,M. Roberts,D. Rodriguez,N. Sasaki,S. R. Schnetzer,L. M. Scott,G. Sinnis,J. D. Smith,P. Sokolsky,C. Song,R. W. Springer,B. T. Stokes,S. Stratton, S. B. Thomas,J. R. Thomas,G. B. Thomson,D. Tupa,A. Zech,X. Zhang Physical Review Letters（2010）
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