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Carvalho W, Rodriguez Cabo I, Rodriguez Fernandez G, Rodriguez Rojo J, Rodriguez-Frias MD, Ros G, Rosado J, Rossler T, Roth M, Roulet E, Rovero AC, Ruehle C, Saffi SJ, Saftoiu A, Salamida F, Salazar H, Greus FS, Salina G, Sanchez F, Sanchez-Lucas P, Santo CE, Santos ED, Santos EM, Sarazin F, Sarkar B, Sarmento R, Sato R, Scharf N, Scherini V, Schieler H, Schiffer P, Schmidt A, Scholten O, Schoorlemmer H, Schovanek P, Schulz A, Schulz J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard RC, Sidelnik I, Sigl G, Sima O, Smialkowski A, Smida R, Snow GR, Sommers P, Sorokin J, Squartini R, Srivastava YN, Stanic S, Stapleton J, Stasielak J, Stephan M, Stutz A, Suarez F, Suomijaervi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Szuba M, Taborda OA, Tapia A, Tartare M, Thao NT, Theodoro VM, Tiffenberg J, Timmermans C, Todero Peixoto CJ, Toma G, Tomankova L, Tome B, Tonachini A, Torralba Elipe G, Machado DT, Travnicek P, Trovato E, Tueros M, Ulrich R, Unger M, Urban M, Valdes Galicia JF, Valino I, Valore L, Van Aar G, Van Den Berg AM, Van Velzen S, Van Vliet A, Varela E, Vargas Cardenas B, Varner G, Vazquez JR, Vazquez RA, Veberic D, Verzi V, Vicha J, Videla M, Villasenor L, Vlcek B, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weidenhaupt K, Weindl A, Werner F, Whelan BJ, Widom A, Wiencke L, Wilczynska B, Wilczynski H, Will M, Williams C, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yamamoto T, Yapici T, Younk P, Yuan G, Yushkov A, Zamorano B, Zas E, Zavrtanik D, Zavrtanik M, Zaw I, Zepeda A, Zhou J, Zhu Y, Silva MZ, Ziolkowski M (2014)
Publication Status: Published
Publication Type: Journal article
Publication year: 2014
Publisher: IOP PUBLISHING LTD
Article Number: ARTN 019
Journal Issue: 8
DOI: 10.1088/1475-7516/2014/08/019
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles greater than 60 degrees detected with the surface array of the Pierre Auger Observatory. The measured signals at the ground level are fitted to muon density distributions predicted with atmospheric cascade models to obtain the relative shower size as an overall normalization parameter. The method is evaluated using simulated showers to test its performance. The energy of the cosmic rays is calibrated using a sub-sample of events reconstructed with both the fluorescence and surface array techniques. The reconstruction method described here provides the basis of complementary analyses including an independent measurement of the energy spectrum of ultra-high energy cosmic rays using very inclined events collected by the Pierre Auger Observatory.
APA:
Aab, A., Abreu, P., Aglietta, M., Ahlers, M., Ahn, E.J., Al Samarai, I.,... Ziolkowski, M. (2014). Reconstruction of inclined air showers detected with the pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics, 8. https://dx.doi.org/10.1088/1475-7516/2014/08/019
MLA:
Aab, A., et al. "Reconstruction of inclined air showers detected with the pierre Auger Observatory." Journal of Cosmology and Astroparticle Physics 8 (2014).
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