The Pierre Auger observatory V: enhancements (2020)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; GOUFFON, PHILIPPE - IF ; TRIDAPALLI, DIOGO BERNARDES - IF
- Unidade: IF
- Subjects: FÍSICA DE ALTA ENERGIA; RAIOS CÓSMICOS; OBSERVATÓRIOS; FÍSICA DE PARTÍCULAS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
-
ABNT
ABREU, P. et al. The Pierre Auger observatory V: enhancements. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/ftp/arxiv/papers/1107/1107.4807.pdf. Acesso em: 12 jan. 2026. , 2020 -
APA
Abreu, P., Albuquerque, I. F. da M. e, Gouffon, P., & Tridapalli, D. B. (2020). The Pierre Auger observatory V: enhancements. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/ftp/arxiv/papers/1107/1107.4807.pdf -
NLM
Abreu P, Albuquerque IF da M e, Gouffon P, Tridapalli DB. The Pierre Auger observatory V: enhancements [Internet]. 2020 ;[citado 2026 jan. 12 ] Available from: https://arxiv.org/ftp/arxiv/papers/1107/1107.4807.pdf -
Vancouver
Abreu P, Albuquerque IF da M e, Gouffon P, Tridapalli DB. The Pierre Auger observatory V: enhancements [Internet]. 2020 ;[citado 2026 jan. 12 ] Available from: https://arxiv.org/ftp/arxiv/papers/1107/1107.4807.pdf - Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger observatory
- Spectral calibration of the fluorescence telescopes of the Pierre Auger observatory
- The Pierre Auger observatory IV: operation and monitoring
- A search for point sources of EeV neutrons
- Features of the energy spectrum of cosmic rays above 2.5×'10 POT. 18' eV using the Pierre Auger observatory
- Reconstruction of events recorded with the surface detector of the Pierre Auger observatory
- Calibration of the underground muon detector of the Pierre Auger observatory
- Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger observatory
- Measurement of the cosmic-ray energy spectrum above 2.5×'10 POT. 18' eV using the Pierre Auger observatory
- Prototype muon detectors for the AMIGA component of the Pierre Auger observatory
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