The Pierre Auger Observatory Upgrade

Giovanni Marsella, A. Aab, P. Abreu, M. Aglietta, E. J. Ahn, I. Al Samarai, I. F.M. Albuquerque, I. Allekotte, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, M. Ambrosio, G. A. Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, F. Arqueros, N. Arsene & 31 others H. Asorey, P. Assis, J. Aublin, G. Avila, A. M. Badescu, A. Balaceanu, C. Baus, J. J. Beatty, K. H. Becker, J. A. Bellido, C. Berat, M. E. Bertaina, X. Bertou, P. L. Biermann, P. Billoir, J. Biteau, S. G. Blaess, A. Blanco, J. Blazek, C. Bleve, M. Boháčová, D. Boncioli, C. Bonifazi, N. Borodai, A. M. Botti, J. Brack, I. Brancus, T. Bretz, A. Bridgeman, G. Farrar, Pierre Auger Collaboration

    Research output: Contribution to journalArticle

    Abstract

    It is planned to operate the Pierre Auger Observatory until at least the end of 2024. An upgrade of the experiment has been proposed in order to provide additional measurements to allow one to elucidate the mass composition and the origin of the flux suppression at the highest energies, to search for a flux contribution of protons up to the highest energies and to reach a sensitivity to a contribution as small as 10% in the flux suppression region, to study extensive air showers and hadronic multi-particle production. With operation planned until 2024, event statistics will more than double compared with the existing Auger data set, with the critical added advantage that every event will now have mass information. Obtaining additional composition-sensitive information will not only help to better reconstruct the properties of the primary particles at the highest energies, but also improve the measurements in the energy range just above the ankle. Furthermore, measurements with the new detectors will help to reduce systematic uncertainties related to the modelling hadronic showers and to limitations in the reconstruction algorithms. A description of the principal proposed Auger upgrade will be presented. The Auger upgrade promises high-quality future data, and real scope for new physics.

    Original languageEnglish (US)
    Article number02003
    JournalEPJ Web of Conferences
    Volume136
    DOIs
    StatePublished - Mar 23 2017

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    observatories
    retarding
    energy
    cosmic ray showers
    particle production
    showers
    statistics
    physics
    protons
    sensitivity
    detectors

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

    Cite this

    Marsella, G., Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Al Samarai, I., ... Pierre Auger Collaboration (2017). The Pierre Auger Observatory Upgrade. EPJ Web of Conferences, 136, [02003]. https://doi.org/10.1051/epjconf/201713602003

    The Pierre Auger Observatory Upgrade. / Marsella, Giovanni; Aab, A.; Abreu, P.; Aglietta, M.; Ahn, E. J.; Al Samarai, I.; Albuquerque, I. F.M.; Allekotte, I.; Allison, P.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J.; Ambrosio, M.; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Arqueros, F.; Arsene, N.; Asorey, H.; Assis, P.; Aublin, J.; Avila, G.; Badescu, A. M.; Balaceanu, A.; Baus, C.; Beatty, J. J.; Becker, K. H.; Bellido, J. A.; Berat, C.; Bertaina, M. E.; Bertou, X.; Biermann, P. L.; Billoir, P.; Biteau, J.; Blaess, S. G.; Blanco, A.; Blazek, J.; Bleve, C.; Boháčová, M.; Boncioli, D.; Bonifazi, C.; Borodai, N.; Botti, A. M.; Brack, J.; Brancus, I.; Bretz, T.; Bridgeman, A.; Farrar, G.; Pierre Auger Collaboration.

    In: EPJ Web of Conferences, Vol. 136, 02003, 23.03.2017.

    Research output: Contribution to journalArticle

    Marsella, G, Aab, A, Abreu, P, Aglietta, M, Ahn, EJ, Al Samarai, I, Albuquerque, IFM, Allekotte, I, Allison, P, Almela, A, Alvarez Castillo, J, Alvarez-Muñiz, J, Ambrosio, M, Anastasi, GA, Anchordoqui, L, Andrada, B, Andringa, S, Aramo, C, Arqueros, F, Arsene, N, Asorey, H, Assis, P, Aublin, J, Avila, G, Badescu, AM, Balaceanu, A, Baus, C, Beatty, JJ, Becker, KH, Bellido, JA, Berat, C, Bertaina, ME, Bertou, X, Biermann, PL, Billoir, P, Biteau, J, Blaess, SG, Blanco, A, Blazek, J, Bleve, C, Boháčová, M, Boncioli, D, Bonifazi, C, Borodai, N, Botti, AM, Brack, J, Brancus, I, Bretz, T, Bridgeman, A, Farrar, G & Pierre Auger Collaboration 2017, 'The Pierre Auger Observatory Upgrade', EPJ Web of Conferences, vol. 136, 02003. https://doi.org/10.1051/epjconf/201713602003
    Marsella G, Aab A, Abreu P, Aglietta M, Ahn EJ, Al Samarai I et al. The Pierre Auger Observatory Upgrade. EPJ Web of Conferences. 2017 Mar 23;136. 02003. https://doi.org/10.1051/epjconf/201713602003
    Marsella, Giovanni ; Aab, A. ; Abreu, P. ; Aglietta, M. ; Ahn, E. J. ; Al Samarai, I. ; Albuquerque, I. F.M. ; Allekotte, I. ; Allison, P. ; Almela, A. ; Alvarez Castillo, J. ; Alvarez-Muñiz, J. ; Ambrosio, M. ; Anastasi, G. A. ; Anchordoqui, L. ; Andrada, B. ; Andringa, S. ; Aramo, C. ; Arqueros, F. ; Arsene, N. ; Asorey, H. ; Assis, P. ; Aublin, J. ; Avila, G. ; Badescu, A. M. ; Balaceanu, A. ; Baus, C. ; Beatty, J. J. ; Becker, K. H. ; Bellido, J. A. ; Berat, C. ; Bertaina, M. E. ; Bertou, X. ; Biermann, P. L. ; Billoir, P. ; Biteau, J. ; Blaess, S. G. ; Blanco, A. ; Blazek, J. ; Bleve, C. ; Boháčová, M. ; Boncioli, D. ; Bonifazi, C. ; Borodai, N. ; Botti, A. M. ; Brack, J. ; Brancus, I. ; Bretz, T. ; Bridgeman, A. ; Farrar, G. ; Pierre Auger Collaboration. / The Pierre Auger Observatory Upgrade. In: EPJ Web of Conferences. 2017 ; Vol. 136.
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    abstract = "It is planned to operate the Pierre Auger Observatory until at least the end of 2024. An upgrade of the experiment has been proposed in order to provide additional measurements to allow one to elucidate the mass composition and the origin of the flux suppression at the highest energies, to search for a flux contribution of protons up to the highest energies and to reach a sensitivity to a contribution as small as 10{\%} in the flux suppression region, to study extensive air showers and hadronic multi-particle production. With operation planned until 2024, event statistics will more than double compared with the existing Auger data set, with the critical added advantage that every event will now have mass information. Obtaining additional composition-sensitive information will not only help to better reconstruct the properties of the primary particles at the highest energies, but also improve the measurements in the energy range just above the ankle. Furthermore, measurements with the new detectors will help to reduce systematic uncertainties related to the modelling hadronic showers and to limitations in the reconstruction algorithms. A description of the principal proposed Auger upgrade will be presented. The Auger upgrade promises high-quality future data, and real scope for new physics.",
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    AU - Marsella, Giovanni

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    AU - Abreu, P.

    AU - Aglietta, M.

    AU - Ahn, E. J.

    AU - Al Samarai, I.

    AU - Albuquerque, I. F.M.

    AU - Allekotte, I.

    AU - Allison, P.

    AU - Almela, A.

    AU - Alvarez Castillo, J.

    AU - Alvarez-Muñiz, J.

    AU - Ambrosio, M.

    AU - Anastasi, G. A.

    AU - Anchordoqui, L.

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    AU - Andringa, S.

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    AU - Arqueros, F.

    AU - Arsene, N.

    AU - Asorey, H.

    AU - Assis, P.

    AU - Aublin, J.

    AU - Avila, G.

    AU - Badescu, A. M.

    AU - Balaceanu, A.

    AU - Baus, C.

    AU - Beatty, J. J.

    AU - Becker, K. H.

    AU - Bellido, J. A.

    AU - Berat, C.

    AU - Bertaina, M. E.

    AU - Bertou, X.

    AU - Biermann, P. L.

    AU - Billoir, P.

    AU - Biteau, J.

    AU - Blaess, S. G.

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