A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger observatory (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:
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ABNT
AAB, A. et al. A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger observatory. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/2010.10953.pdf. Acesso em: 15 maio 2024. , 2020 -
APA
Aab, A., Albuquerque, I. F. da M. e, Gouffon, P., & Tridapalli, D. B. (2020). A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger observatory. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/2010.10953.pdf -
NLM
Aab A, Albuquerque IF da M e, Gouffon P, Tridapalli DB. A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger observatory [Internet]. 2020 ;[citado 2024 maio 15 ] Available from: https://arxiv.org/pdf/2010.10953.pdf -
Vancouver
Aab A, Albuquerque IF da M e, Gouffon P, Tridapalli DB. A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger observatory [Internet]. 2020 ;[citado 2024 maio 15 ] Available from: https://arxiv.org/pdf/2010.10953.pdf - Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory
- Large-scale distribution of arrival directions of cosmic rays detected above `10 POT.18´ eV at the Pierre auger Observatory
- 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
- Studies on the response of a water-cherenkov detector of the Pierre Auger observatory to atmospheric muons using an RPC hodoscope
- Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers
- Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory
- Cosmic-ray anisotropies in right ascension measured by the Pierre Auger observatory
- Features of the energy spectrum of cosmic rays above 2.5×'10 POT. 18' eV using the Pierre Auger observatory
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