Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger observatory (2016)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; GOUFFON, PHILIPPE - IF
- Unidade: IF
- Subjects: ENERGIA; RAIOS CÓSMICOS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
-
ABNT
AAB, A. e ALBUQUERQUE, Ivone Freire da Mota e e GOUFFON, Philippe. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger observatory. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/1608.07378.pdf. Acesso em: 08 jun. 2024. , 2016 -
APA
Aab, A., Albuquerque, I. F. da M. e, & Gouffon, P. (2016). Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger observatory. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/1608.07378.pdf -
NLM
Aab A, Albuquerque IF da M e, Gouffon P. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger observatory [Internet]. 2016 ;[citado 2024 jun. 08 ] Available from: https://arxiv.org/pdf/1608.07378.pdf -
Vancouver
Aab A, Albuquerque IF da M e, Gouffon P. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger observatory [Internet]. 2016 ;[citado 2024 jun. 08 ] Available from: https://arxiv.org/pdf/1608.07378.pdf - The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory
- The pierre auger observatory I: the cosmic ray energy spectrum and related measurements
- Description of atmospheric conditions at the pierre auger observatory using the global data assimilation system (gdas)
- Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy
- The pierre auger observatory V: enhancements
- The pierre auger observatory II: studies of cosmic ray composition and hadronic interaction models
- Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory
- Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
- Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the pierre auger observatory
- Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory
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