{"paper":{"title":"Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A. Almela, A.A. Watson, A. Bakalova, A. Balaceanu, A. Blanco, A. Bridgeman, A. Bueno, A. Cancio, A. Castellina, A.C. Cobos Cerutti, A.C. Fauth, A. Coleman, A. Condorelli, A.C. Rovero, A.D. Supanitsky, A. Dundovic, A. Etchegoyen, A. Filip\\v{c}i\\v{c}, A. Fuster, A. Gherghel-Lascu, A.G. Mariazzi, A. Gorgi, A. Haungs, A. Insolia, A. K\\\"a\\\"ap\\\"a, A. Kuotb Awad, A. Letessier-Selvon, A.L. M\\\"uller, A. L\\'opez Casado, A. Lucero, A.M. Badescu, A.M. Botti, A. Menshikov, A.M. van den Berg, A Nucita, A. Olinto, A. Parra, A. Puyleart, A. Saftoiu, A. Streich, A. Taboada, A. Tapia, A. Travaini, A. van Vliet, A. Weindl, A. Yushkov, A. Zepeda, B. Andrada, B.C. Manning, B. Daniel, B. Garc\\'ia, B. Keilhauer, B.L. Lago, B. Mitrica, B. Pont, B.R. Dawson, B. Tom\\'e, B. Vargas C\\'ardenas, B. Wundheiler, B. Zimmermann, C. Aramo, C. Berat, C. Bleve, C. Bonifazi, C. Dobrigkeit, C.E. Covault, C. Hojvat, C.J. Todero Peixoto, C. Morello, C.O. Escobar, C. Peters, C. Porowski, C. Sarmiento-Cano, C. Timmermans, C. Ventura, D. Boncioli, D. G{\\l}as, D. G\\'ora, D. Harari, D. Heck, D. Kuempel, D. LaHurd, D. Lo Presti, D. Mandat, D. Martello, D. Melo, D. Mockler, D. Nitz, D. Nosek, D. Ravignani, D. Schmidt, D. Stanca, D. Veberi\\v{c}, D. Wittkowski, D. Zavrtanik, E. Guido, E. Mayotte, E.M. Holt, E.M. Santos, E. Roulet, E. Santos, E. Varela, E. Zas, F. Barbato, F. Canfora, F. Catalani, F. Contreras, F. Convenga, F. Diogo, F. Feldbusch, F. Fenu, F. Gobbi, F.G. Schr\\\"oder, F. Guarino, F.L. Briechle, F. Montanet, F.O. de Oliveira Salles, F. Pedreira, F. Riehn, F. Salamida, F. S\\'anchez, F. Sarazin, F. Schl\\\"uter, F. Suarez, F. Zuccarello, G.A. Anastasi, G. Avila, G. Cataldi, G.C. Hill, G. Consolati, G. De Mauro, G. Farrar, G. Golup, G. Kukec Mezek, G. Mancarella, G. Marsella, G. Matthiae, G. Medina-Tanco, G. Morlino, G. Parente, G.P. Guedes, G.R. Snow, G. Salina, G. Sigl, G. Silli, G. Torralba Elipe, H. Asorey, H. Falcke, H. Gemmeke, H.J. Mathes, H. Martinez, H.O. Klages, H. Salazar, H. Schieler, H. Wahlberg, H. Wilczy\\'nski, I. Allekotte, I.C. Mari\\c{s}, I. De Mitri, I.D. Vergara Quispe, I.F.M. Albuquerque, I. Goos, I. Jandt, I. Lhenry-Yvon, I. Vali\\~no, J.A. Bellido, J.A. Chinellato, J.A. Day, J.A. Johnsen, J. Alvarez Castillo, J. Alvarez-Mu\\~niz, J. Biteau, J. Blazek, J. Brack, J.C. D'Olivo, J. Chudoba, J. Debatin, J. de Oliveira, J.D. Sanabria Gomez, J. Ebr, J. Farmer, J.F. Soriano, J.F. Vald\\'es Galicia, J. Glombitza, J. Hulsman, J. Jurysek, J. Kemp, J. Kleinfeller, J.M. Albury, J. Matthews, J.M. Carceller, J.M. Figueira, J. Pallotta, J. Pe\\~na-Rodriguez, J.P. Gongora, J. Phuntsok, J. P\\k{e}kala, J. Poh, J. Rautenberg, J.R. H\\\"orandel, J. Ridky, J. Rodriguez Rojo, J.R.T. de Mello Neto, J. Schumacher, J. Souchard, J. Stasielak, J. Vicha, J. Vink, J. \\v{S}up\\'ik, K. Daumiller, K.-D. Merenda, K.H. Becker, K.H. Kampert, K.S. Caballero-Mora, L. Anchordoqui, L.A. N\\'u\\~nez, L.A.S. Pereira, L. Caccianiga, L. Calcagni, L. Cazon, L. Chytka, L. Lopes, L. Middendorf, L. Miramonti, L. Nellen, L. No\\v{z}ka, L. Perrone, L.P. Ferreyro, L. Valore, L. Villase\\~nor, L. Wiencke, L. Yang, L. Zehrer, M. Aglietta, M.A. Leigui de Oliveira, M.A. Muller, M. Boh\\'a\\v{c}ov\\'a, M. Buscemi, M. Cerda, M. del R\\'io, M.E. Bertaina, M. Erdmann, M. Giammarchi, M. Giller, M. G\\'omez Berisso, M. Gottowik, M. Hrabovsk\\'y, M.I. Micheletti, M.J. Cooper, M. Josebachuili, M.J. Roncoroni, M. Kleifges, M.L. D\\'iaz Castro, M. Malacari, M. Mastrodicasa, M.M. Freire, M. Mostaf\\'a, M. Niculescu-Oglinzanu, M. Niechciol, M. Palatka, M. Pech, M. Perlin, M. Pimenta, M. Platino, M.P. Panetta, M. Prouza, M.R. Coluccia, M. Reininghaus, M.R. Hampel, M. Risse, M. Roth, M. Schauer, M. Schimassek, M. Schimp, M. Scornavacche, M. Stolpovskiy, M. Su\\'arez-Dur\\'an, M.T. Dova, M. Trini, M. Tueros, M. Unger, M. Urban, M. Weber, M. Wiede\\'nski, M. Wirtz, M. Zavrtanik, M. Ziolkowski, N. Borodai, N. Dhital, N. Fazzini, N. Gonz\\'alez, N. Kemmerich, O.A. Taborda, O.C. Lippmann, O. Deligny, O. Mart\\'inez Bravo, O. Scholten, O. Sima, P. Abreu, P. Assis, P. Buchholz, P.F. G\\'omez Vitale, P.G. Isar, P. Hansen, P. Heimann, P.H. Nguyen, P. Homola, P. Horvath, P.L. Biermann, P.L. Ghia, P. Mantsch, P.O. Mazur, P. Papenbreer, P. Privitera, P. Ristori, P. Ruehl, P. Savina, P. Schov\\'anek, P. Sommers, P. Stassi, P. Travnicek, P. van Bodegom, Q. Dorosti, Q. Luce, R. Caruso, R.C. dos Anjos, R. Colalillo, R. Concei\\c{c}\\~ao, R.C. Shellard, R. Engel, R.G. Lang, R. Halliday, R.J. Barreira Luz, R. Krause, R. Legumina, R. L\\'opez, R. Lorek, R.M. de Almeida, R. Mussa, R. Pelayo, R. Ramos-Pollan, R.R. Prado, R. Sarmento, R. Sato, R. Squartini, R. Ulrich, R. \\v{S}m\\'ida, R.W. Clay, S. Andringa, S. Baur, S. Buitink, S. Coutu, S. Dasso, S.G. Blaess, S.J. De Jong, S.J. Saffi, S.J. Sciutto, S. Mathys, S. Michal, S. Mollerach, S. M\\\"uller, S. Petrera, S. Querchfeld, S. Quinn, S. Schr\\\"oder, S. Stani\\v{c}, S. Vorobiov, T.A. Harrison, T. Bretz, T.D. Grubb, T. Fujii, T. Hebbeker, The Pierre Auger Collaboration: A. Aab, T. Huege, T. Pierog, T. Sudholz, T. Suomij\\\"arvi, T. Winchen, U. Giaccari, V. de Souza, V. Lenok, V.M. Harvey, V. Novotny, V. Pirronello, V. Rizi, V. Scherini, V. Verzi, W. Rodrigues de Carvalho, X. Bertou, Z. Szadkowski, Z. Zong","submitted_at":"2019-01-23T18:46:53Z","abstract_excerpt":"The determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it al"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.08040","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1901.08040/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}