The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory (2011)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; GOUFFON, PHILIPPE - IF ; CARVALHO JUNIOR, WASHINGTON RODRIGUES DE - IF ; PEIXOTO, CARLOS JOSÉ TODERO - IFSC ; TRIDAPALLI, DIOGO BERNARDES - IF
- Unidades: IF; IFSC
- DOI: 10.1016/j.astropartphys.2011.08.001
- Subjects: FÍSICA DE PARTÍCULAS; MÉTODO DE MONTE CARLO; RAIOS CÓSMICOS
- Language: Inglês
- Imprenta:
- Source:
- Título: Astroparticle Physics
- ISSN: 0927-6505
- Volume/Número/Paginação/Ano: v. 35, n. 5, p. 266-276, Dec. 2011
- Status:
- Artigo possui acesso gratuito no site do editor (Bronze Open Access)
- Versão do Documento:
- Versão publicada (Published version)
- Acessar versão aberta:
-
ABNT
ABREU, P. et al. The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory. Astroparticle Physics, v. 35, n. 5, p. 266-276, 2011Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2011.08.001. Acesso em: 13 abr. 2026. -
APA
Abreu, P., Albuquerque, I. F. da M. e, Souza, V. de, Gouffon, P., Carvalho, W. R. de, Peixoto, C. J. T., & Tridapalli, D. B. (2011). The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory. Astroparticle Physics, 35( 5), 266-276. doi:10.1016/j.astropartphys.2011.08.001 -
NLM
Abreu P, Albuquerque IF da M e, Souza V de, Gouffon P, Carvalho WR de, Peixoto CJT, Tridapalli DB. The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory [Internet]. Astroparticle Physics. 2011 ; 35( 5): 266-276.[citado 2026 abr. 13 ] Available from: https://doi.org/10.1016/j.astropartphys.2011.08.001 -
Vancouver
Abreu P, Albuquerque IF da M e, Souza V de, Gouffon P, Carvalho WR de, Peixoto CJT, Tridapalli DB. The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory [Internet]. Astroparticle Physics. 2011 ; 35( 5): 266-276.[citado 2026 abr. 13 ] Available from: https://doi.org/10.1016/j.astropartphys.2011.08.001 - Erratum to “The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory” [Astroparticle Physics 35 (2011) 266–276]
- Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
- Search for point-like sources of ultra-high energy neutrinos at the Pierre Auger observatory and improved limit on the diffuse flux of tau neutrinos
- The rapid atmospheric monitoring system of the Pierre Auger Observatory
- A search for point sources of EeV neutrons
- Techniques for measuring aerosol attenuation using the Central Laser Facility at the Pierre Auger Observatory
- Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory
- Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory
- Constraints on the origin of cosmic rays above '10 POT. 18' eV from large-scale anisotropy searches in data of the Pierre Auger observatory
- Large-scale distribution of arrival directions of cosmic rays detected above '10 POT. 18' eV at the Pierre Auger Observatory
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