Pierre Auger observatory and telescope array: joint contributions to the 34th international cosmic ray conference (ICRC 2015) (2015)
- Autores:
- Autores USP: SANTOS, EDIVALDO MOURA - IF ; ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; GOUFFON, PHILIPPE - IF
- Unidade: IF
- Assuntos: NEUTRINO; REAÇÕES NUCLEARES; ACELERADOR DE PARTÍCULAS
- Idioma: Inglês
- Imprenta:
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ABNT
AAB, A et al. Pierre Auger observatory and telescope array: joint contributions to the 34th international cosmic ray conference (ICRC 2015). . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: http://arxiv.org/pdf/1511.02103v1.pdf. Acesso em: 24 abr. 2024. , 2015 -
APA
Aab, A., Santos, E. M., Albuquerque, I. F. da M. e, & Gouffon, P. (2015). Pierre Auger observatory and telescope array: joint contributions to the 34th international cosmic ray conference (ICRC 2015). São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de http://arxiv.org/pdf/1511.02103v1.pdf -
NLM
Aab A, Santos EM, Albuquerque IF da M e, Gouffon P. Pierre Auger observatory and telescope array: joint contributions to the 34th international cosmic ray conference (ICRC 2015) [Internet]. 2015 ;[citado 2024 abr. 24 ] Available from: http://arxiv.org/pdf/1511.02103v1.pdf -
Vancouver
Aab A, Santos EM, Albuquerque IF da M e, Gouffon P. Pierre Auger observatory and telescope array: joint contributions to the 34th international cosmic ray conference (ICRC 2015) [Internet]. 2015 ;[citado 2024 abr. 24 ] Available from: http://arxiv.org/pdf/1511.02103v1.pdf - An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger observatory
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- Measurement of the cosmic ray spectrum above 4x'10 POT. 18' eV using inclined events detected with the Pierre Auger observatory
- Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers
- The Pierre Auger observatory: contributions to the 34th international cosmic ray conference (ICRC 2015)
- Energy estimation of cosmic rays with the engineering radio array of the Pierre Auger observatory
- Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-cherenkov detectors of the Pierre Auger observatory
- Observation of a large-scale anisotropy in the arrival directions of cosmic rays above '8×10 POT. 18' eV
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