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@ARTICLE{Aguilar:891400,
      author       = {Aguilar, M. and Cavasonza, L. Ali and Allen, M. S. and
                      Alpat, B. and Ambrosi, G. and Arruda, L. and Attig, N. and
                      Barao, F. and Barrin, L. and Bartoloni, A. and Başeğmez-du
                      Pree, S. and Battiston, R. and Behlmann, M. and Beischer, B.
                      and Berdugo, J. and Bertucci, B. and Bindi, V. and de Boer,
                      W. and Bollweg, K. and Borgia, B. and Boschini, M. J. and
                      Bourquin, M. and Bueno, E. F. and Burger, J. and Burger, W.
                      J. and Burmeister, S. and Cai, X. D. and Capell, M. and
                      Casaus, J. and Castellini, G. and Cervelli, F. and Chang, Y.
                      H. and Chen, G. M. and Chen, G. R. and Chen, H. S. and Chen,
                      Y. and Cheng, L. and Chou, H. Y. and Chouridou, S. and
                      Choutko, V. and Chung, C. H. and Clark, C. and Coignet, G.
                      and Consolandi, C. and Contin, A. and Corti, C. and Cui, Z.
                      and Dadzie, K. and Delgado, C. and Della Torre, S. and
                      Demirköz, M. B. and Derome, L. and Di Falco, S. and Di
                      Felice, V. and Díaz, C. and Dimiccoli, F. and von
                      Doetinchem, P. and Dong, F. and Donnini, F. and Duranti, M.
                      and Egorov, A. and Eline, A. and Feng, J. and Fiandrini, E.
                      and Fisher, P. and Formato, V. and Freeman, C. and
                      Galaktionov, Y. and Gámez, C. and García-López, R. J. and
                      Gargiulo, C. and Gast, H. and Gervasi, M. and Giovacchini,
                      F. and Gómez-Coral, D. M. and Gong, J. and Goy, C. and
                      Grabski, V. and Grandi, D. and Graziani, M. and Haino, S.
                      and Han, K. C. and Hashmani, R. K. and He, Z. H. and Heber,
                      B. and Hsieh, T. H. and Hu, J. Y. and Incagli, M. and Jang,
                      W. Y. and Jia, Yi and Jinchi, H. and Kanishev, K. and
                      Khiali, B. and Kim, G. N. and Kirn, Th. and Konyushikhin, M.
                      and Kounina, O. and Kounine, A. and Koutsenko, V. and
                      Kuhlman, A. and Kulemzin, A. and La Vacca, G. and Laudi, E.
                      and Laurenti, G. and Lazzizzera, I. and Lebedev, A. and Lee,
                      H. T. and Lee, S. C. and Li, J. Q. and Li, M. and Li, Q. and
                      Li, S. and Li, J. H. and Li, Z. H. and Liang, J. and Light,
                      C. and Lin, C. H. and Lippert, T. and Liu, J. H. and Liu, Z.
                      and Lu, S. Q. and Lu, Y. S. and Luebelsmeyer, K. and Luo, J.
                      Z. and Luo, Xi and Lyu, S. S. and Machate, F. and Mañá, C.
                      and Marín, J. and Marquardt, J. and Martin, T. and
                      Martínez, G. and Masi, N. and Maurin, D. and
                      Menchaca-Rocha, A. and Meng, Q. and Mikhailov, V. V. and Mo,
                      D. C. and Molero, M. and Mott, P. and Mussolin, L. and
                      Negrete, J. and Nikonov, N. and Nozzoli, F. and Oliva, A.
                      and Orcinha, M. and Palermo, M. and Palmonari, F. and
                      Paniccia, M. and Pashnin, A. and Pauluzzi, M. and Pensotti,
                      S. and Phan, H. D. and Piandani, R. and Plyaskin, V. and
                      Poluianov, S. and Qin, X. and Qu, Z. Y. and Quadrani, L. and
                      Rancoita, P. G. and Rapin, D. and Conde, A. Reina and Robyn,
                      E. and Rosier-Lees, S. and Rozhkov, A. and Rozza, D. and
                      Sagdeev, R. and Schael, S. and von Dratzig, A. Schulz and
                      Schwering, G. and Seo, E. S. and Shakfa, Z. and Shan, B. S.
                      and Siedenburg, T. and Solano, C. and Song, J. W. and Song,
                      X. J. and Sonnabend, R. and Strigari, L. and Su, T. and Sun,
                      Q. and Sun, Z. T. and Tacconi, M. and Tang, X. W. and Tang,
                      Z. C. and Tian, J. and Ting, Samuel C. C. and Ting, S. M.
                      and Tomassetti, N. and Torsti, J. and Tüysüz, C. and
                      Urban, T. and Usoskin, I. and Vagelli, V. and Vainio, R. and
                      Valencia-Otero, M. and Valente, E. and Valtonen, E. and
                      Vázquez Acosta, M. and Vecchi, M. and Velasco, M. and
                      Vialle, J. P. and Wang, C. X. and Wang, L. and Wang, L. Q.
                      and Wang, N. H. and Wang, Q. L. and Wang, S. and Wang, X.
                      and Wang, Yu and Wang, Z. M. and Wei, J. and Weng, Z. L. and
                      Wu, H. and Xiong, R. Q. and Xu, W. and Yan, Q. and Yang, Y.
                      and Yashin, I. I. and Yi, H. and Yu, Y. M. and Yu, Z. Q. and
                      Zannoni, M. and Zhang, C. and Zhang, F. and Zhang, F. Z. and
                      Zhang, J. H. and Zhang, Z. and Zhao, F. and Zheng, C. and
                      Zheng, Z. M. and Zhuang, H. L. and Zhukov, V. and Zichichi,
                      A. and Zimmermann, N. and Zuccon, P.},
      title        = {{P}roperties of {I}ron {P}rimary {C}osmic {R}ays: {R}esults
                      from the {A}lpha {M}agnetic {S}pectrometer},
      journal      = {Physical review letters},
      volume       = {126},
      number       = {4},
      issn         = {1079-7114},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {FZJ-2021-01488},
      pages        = {041104},
      year         = {2021},
      abstract     = {We report the observation of new properties of primary iron
                      (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV
                      with 0.62×106 iron nuclei collected by the Alpha Magnetic
                      Spectrometer experiment on the International Space Station.
                      Above 80.5 GV the rigidity dependence of the cosmic ray Fe
                      flux is identical to the rigidity dependence of the primary
                      cosmic ray He, C, and O fluxes, with the Fe/O flux ratio
                      being constant at 0.155±0.006. This shows that unexpectedly
                      Fe and He, C, and O belong to the same class of primary
                      cosmic rays which is different from the primary cosmic rays
                      Ne, Mg, and Si class.},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {512 - Supercomputing $\&$ Big Data Infrastructures
                      (POF4-512)},
      pid          = {G:(DE-HGF)POF4-512},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {33576661},
      UT           = {WOS:000612682500002},
      doi          = {10.1103/PhysRevLett.126.041104},
      url          = {https://juser.fz-juelich.de/record/891400},
}