Artículo

Ros, G.; Supanitsky, A.D.; Medina-Tanco, G.A.; Del Peral, L.; Rodríguez-Frías, M.D. "Improving photon-hadron discrimination based on cosmic ray surface detector data" (2013) Astroparticle Physics. 47:10-17
Estamos trabajando para incorporar este artículo al repositorio
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

The search for photons at EeV energies and beyond has considerable astrophysical interest and will remain one of the key challenges for ultra-high energy cosmic ray (UHECR) observatories in the near future. Several upper limits to the photon flux have been established since no photon has been unambiguously observed up to now. An improvement in the reconstruction efficiency of the photon showers and/or better discrimination tools are needed to improve these limits apart from an increase in statistics. Following this direction, we analyze in this work the ability of the surface parameter Sb, originally proposed for hadron discrimination, for photon search. Semi-analytical and numerical studies are performed in order to optimize S b for the discrimination of photons from a proton background in the energy range from 1018.5 to 1019.6 eV. Although not shown explicitly, the same analysis has been performed for Fe nuclei and the corresponding results are discussed when appropriate. The effects of different array geometries and the underestimation of the muon component in the shower simulations are analyzed, as well as the Sb dependence on primary energy and zenith angle. © 2013 Elsevier B.V. All rights reserved.

Registro:

Documento: Artículo
Título:Improving photon-hadron discrimination based on cosmic ray surface detector data
Autor:Ros, G.; Supanitsky, A.D.; Medina-Tanco, G.A.; Del Peral, L.; Rodríguez-Frías, M.D.
Filiación:Space and Astroparticle Group, Dpto. Física y Matemáticas, Universidad de Alcalá, Ctra. Madrid-Barcelona km. 33, Alcalá de Henares E-28871, Spain
Instituto de Astronomía y Física del Espacio, IAFE, CONICET-UBA, Argentina
Instituto de Ciencias Nucleares, UNAM, Circuito Exteriror S/N, Ciudad Universitaria, Mexico D. F. 04510, Mexico
Palabras clave:Cherenkov detectors; Cosmic rays; Photon discrimination; Sb parameter; Array geometries; Cherenkov Detectors; Photon discrimination; Primary energies; Reconstruction efficiency; Sb parameter; Surface parameter; Ultrahigh-energy cosmic rays; Cosmic rays; Hadrons; Photons
Año:2013
Volumen:47
Página de inicio:10
Página de fin:17
DOI: http://dx.doi.org/10.1016/j.astropartphys.2013.05.014
Título revista:Astroparticle Physics
Título revista abreviado:Astropart. Phys.
ISSN:09276505
CODEN:APHYE
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09276505_v47_n_p10_Ros

Referencias:

  • Gelmini, G., Kalashev, O., Semikoz, D.V., (2008) J. Exp. Theor. Phys., 106, pp. 1061-1082
  • Hayashida, N., (1994) Phys. Rev. Lett., 73, p. 3491
  • Bhattacharjee, P., Sigl, G., (2000) Phys. Rep., 327, pp. 109-247. , arxiv:astro-ph/9811011
  • (2010) Phys. Lett. B, 685, pp. 239-246. , The Pierre Auger Collaboration
  • Zhang, B., (2008) Nucl. Phys. Proc. Suppl., 175-176, pp. 241-244
  • Shinozaki, K., (2002) Astrophys. J., 571, pp. L117
  • Glushkov, A.V., (2010) Phys. Rev., D82, p. 041101
  • (2008) Astropart. Phys., 29, pp. 243-256. , The Pierre Auger Collaboration
  • Rubtsov, G., (2011) Proc. 32nd ICRC, , [Telescope Array Collaboration Beijing, China
  • Settimo, M., (2011) Proc. 32nd ICRC, , arxiv:1107.4805 the Pierre Auger Collaboration Beijing, China
  • Alvarez-Muniz, J., Risse, M., (2012) UHECR International Symposium, , [Pierre Auger Collaboration], G.I. Rubtsov, B.T. Stokes [Telescope Array Collaboration] CERN. EPJ Web of Conferences
  • Busca, N., Hooper, D., Kolb, E.W., (2006) Phys. Rev. D, 73, p. 123001. , arxiv:astro-ph/0603055
  • (2012) Phys. Rev. Lett., p. 062002. , The Pierre Auger Collaboration
  • (2010) Phys. Rev. Lett., 104, p. 091101. , The Pierre Auger Collaboration
  • Ros, G., (2011) Astropart. Phys., 35, p. 140
  • Telescope Array Collaboration. arXiv:1205.5067; P. Billoir, C. Roucelle, J.C. Hamilton. arXiv:astro-ph/0701583; Greisen, K., (1956) Prog. Cosmic Ray Phys., 3
  • Ostapchenko, S., (2006) Nucl. Phys. Proc. Suppl., B151, p. 143
  • Ros, G., (2009) Nucl. Instrum. Methods, A608, p. 454
  • Engel, R., (2007) Proc. of 30th ICRC, , arxiv:0706.1921, the Pierre Auger Collaboration Mérida, México
  • Castellina, A., (2009) Proc. of 31st ICRC, , arxiv:0906.2319, the Pierre Auger Collaboration Łódź, Poland
  • Allen, J., (2011) Proc. 32nd ICRC, , arxiv:1107.4804 the Pierre Auger Collaboration Beijing, China
  • http://www.fisica.unlp.edu.ar/auger/aires, S. Sciutto, 1999. arxiv:astro-ph/9911331; Engel, R., (1999) Proc. 26th ICRC, 1, p. 415. , Salt Lake City (USA)
  • Argiró, S., (2007) Nucl. Instrum. Methods, A580, pp. 1485-1496
  • Badagnani, D., Sciutto, S.J., (2005) Proc. of 29th ICRC, , Pune, India
  • Homola, P., (2007) Astropart. Phys., 27, pp. 174-184

Citas:

---------- APA ----------
Ros, G., Supanitsky, A.D., Medina-Tanco, G.A., Del Peral, L. & Rodríguez-Frías, M.D. (2013) . Improving photon-hadron discrimination based on cosmic ray surface detector data. Astroparticle Physics, 47, 10-17.
http://dx.doi.org/10.1016/j.astropartphys.2013.05.014
---------- CHICAGO ----------
Ros, G., Supanitsky, A.D., Medina-Tanco, G.A., Del Peral, L., Rodríguez-Frías, M.D. "Improving photon-hadron discrimination based on cosmic ray surface detector data" . Astroparticle Physics 47 (2013) : 10-17.
http://dx.doi.org/10.1016/j.astropartphys.2013.05.014
---------- MLA ----------
Ros, G., Supanitsky, A.D., Medina-Tanco, G.A., Del Peral, L., Rodríguez-Frías, M.D. "Improving photon-hadron discrimination based on cosmic ray surface detector data" . Astroparticle Physics, vol. 47, 2013, pp. 10-17.
http://dx.doi.org/10.1016/j.astropartphys.2013.05.014
---------- VANCOUVER ----------
Ros, G., Supanitsky, A.D., Medina-Tanco, G.A., Del Peral, L., Rodríguez-Frías, M.D. Improving photon-hadron discrimination based on cosmic ray surface detector data. Astropart. Phys. 2013;47:10-17.
http://dx.doi.org/10.1016/j.astropartphys.2013.05.014