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Artigo de periodico
Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer (2019)
Aguilar, M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, ISÓTOPOS, ESPECTROMETRIA
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ABNT
AGUILAR, M. e VECCHI, Manuela. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer. Physical Review Letters, v. No 2019, n. 18, p. 181102-1-181102-8, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.123.181102. Acesso em: 14 set. 2024.
APA
Aguilar, M., & Vecchi, M. (2019). Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer. Physical Review Letters, No 2019( 18), 181102-1-181102-8. doi:10.1103/PhysRevLett.123.181102
NLM
Aguilar M, Vecchi M. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer [Internet]. Physical Review Letters. 2019 ; No 2019( 18): 181102-1-181102-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.123.181102
Vancouver
Aguilar M, Vecchi M. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer [Internet]. Physical Review Letters. 2019 ; No 2019( 18): 181102-1-181102-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.123.181102
Artigo de periodico
Towards understanding the origin of cosmic-ray positrons (2019)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, v. 122, n. 4, p. 041102-1-041102-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.041102. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, 122( 4), 041102-1-041102-9. doi:10.1103/PhysRevLett.122.041102
NLM
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
Vancouver
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
Artigo de periodico
Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation (2019)
Genolini, Y.; Boudaud, M.; Batista, P-I.; Caroff, S.; Derome, L.; Lavalle, J.; Marcowith, A.; Maurin, D.; Poireau, V.; Poulin, V.; Rosier, S.; Salati, P.; Serpico, P. D.; Vecchi, Manuela
Source: Physical Review D. Unidade: IFSC
Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
GENOLINI, Y. et al. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation. Physical Review D, v. 99, n. 12, p. 123028-1-123028-16, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.99.123028. Acesso em: 14 set. 2024.
APA
Genolini, Y., Boudaud, M., Batista, P. -I., Caroff, S., Derome, L., Lavalle, J., et al. (2019). Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation. Physical Review D, 99( 12), 123028-1-123028-16. doi:10.1103/PhysRevD.99.123028
NLM
Genolini Y, Boudaud M, Batista P-I, Caroff S, Derome L, Lavalle J, Marcowith A, Maurin D, Poireau V, Poulin V, Rosier S, Salati P, Serpico PD, Vecchi M. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation [Internet]. Physical Review D. 2019 ; 99( 12): 123028-1-123028-16.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028
Vancouver
Genolini Y, Boudaud M, Batista P-I, Caroff S, Derome L, Lavalle J, Marcowith A, Maurin D, Poireau V, Poulin V, Rosier S, Salati P, Serpico PD, Vecchi M. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation [Internet]. Physical Review D. 2019 ; 99( 12): 123028-1-123028-16.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028
Trabalho de evento-anais periodico
Multimessenger astrophysics: session summary (2019)
Ahlers, Markus; Vecchi, Manuela
Source: Proceedings of Science. Conference titles: Neutrino Oscillation Workshop - NOW. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AHLERS, Markus e VECCHI, Manuela. Multimessenger astrophysics: session summary. Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. Disponível em: https://doi.org/10.22323/1.337.0059. Acesso em: 14 set. 2024. , 2019
APA
Ahlers, M., & Vecchi, M. (2019). Multimessenger astrophysics: session summary. Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. doi:10.22323/1.337.0059
NLM
Ahlers M, Vecchi M. Multimessenger astrophysics: session summary [Internet]. Proceedings of Science. 2019 ; 337 059-1-059-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.22323/1.337.0059
Vancouver
Ahlers M, Vecchi M. Multimessenger astrophysics: session summary [Internet]. Proceedings of Science. 2019 ; 337 059-1-059-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.22323/1.337.0059
Artigo de periodico
Towards understanding the origin of cosmic-ray electrons (2019)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, v. 122, n. 10, p. 101101-1-101101-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.101101. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, 122( 10), 101101-1-101101-9. doi:10.1103/PhysRevLett.122.101101
NLM
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
Vancouver
Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
Monografia/livro
Science with the Cherenkov Telescope Array: the CTA Consortium (2019)
Souza, Vitor de ; Vecchi, Manuela ; Peixoto, Carlos Jose Todero ; Catalani, Fernando; Dal Pino, Elisabete Maria de Gouveia; Lang, Rodrigo Guedes; Falceta Gonçalves, Diego Antonio
Unidades: IFSC, EEL, IAG, EACH
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, FÍSICA DE ALTA ENERGIA
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ABNT
SOUZA, Vitor de et al. Science with the Cherenkov Telescope Array: the CTA Consortium. . Singapore: World Scientific Publishing. . Acesso em: 14 set. 2024. , 2019
APA
Souza, V. de, Vecchi, M., Peixoto, C. J. T., Catalani, F., Dal Pino, E. M. de G., Lang, R. G., & Falceta Gonçalves, D. A. (2019). Science with the Cherenkov Telescope Array: the CTA Consortium. Singapore: World Scientific Publishing.
NLM
Souza V de, Vecchi M, Peixoto CJT, Catalani F, Dal Pino EM de G, Lang RG, Falceta Gonçalves DA. Science with the Cherenkov Telescope Array: the CTA Consortium. 2019 ;[citado 2024 set. 14 ]
Vancouver
Souza V de, Vecchi M, Peixoto CJT, Catalani F, Dal Pino EM de G, Lang RG, Falceta Gonçalves DA. Science with the Cherenkov Telescope Array: the CTA Consortium. 2019 ;[citado 2024 set. 14 ]
Artigo de periodico
Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout (2019)
Acharyya, A.; Souza, Vitor de ; Vecchi, Manuela; Dal Pino, Elisabete Maria de Gouveia; Kowal, Grzegorz
Source: Astroparticle Physics. Unidades: IFSC, EACH, IAG
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, FÍSICA DE ALTA ENERGIA
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ABNT
ACHARYYA, A. et al. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout. Astroparticle Physics, v. 111, p. 35-53, 2019Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2019.04.001. Acesso em: 14 set. 2024.
APA
Acharyya, A., Souza, V. de, Vecchi, M., Dal Pino, E. M. de G., & Kowal, G. (2019). Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout. Astroparticle Physics, 111, 35-53. doi:10.1016/j.astropartphys.2019.04.001
NLM
Acharyya A, Souza V de, Vecchi M, Dal Pino EM de G, Kowal G. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout [Internet]. Astroparticle Physics. 2019 ; 111 35-53.[citado 2024 set. 14 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.04.001
Vancouver
Acharyya A, Souza V de, Vecchi M, Dal Pino EM de G, Kowal G. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout [Internet]. Astroparticle Physics. 2019 ; 111 35-53.[citado 2024 set. 14 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.04.001
Artigo de periodico
Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. et al. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051101-1-051101-7, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051101. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051101-1-051101-7. doi:10.1103/PhysRevLett.121.051101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
Artigo de periodico
Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. et al. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051102-1-051102-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051102. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051102-1-051102-8. doi:10.1103/PhysRevLett.121.051102
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
Curadoria
South American Dark Matter Workshop, 2 (2018)
Bertuzzo, Enrico (cur); Vecchi, Manuela (cur)
Unidades: IF, IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ASTROFÍSICA
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ABNT
South American Dark Matter Workshop, 2. . São Paulo: International Centre for Theoretical Physics, ICTP, South American Institute for Fundamental Research, SAIFR. . Acesso em: 14 set. 2024. , 2018
APA
South American Dark Matter Workshop, 2. (2018). South American Dark Matter Workshop, 2. São Paulo: International Centre for Theoretical Physics, ICTP, South American Institute for Fundamental Research, SAIFR.
NLM
South American Dark Matter Workshop, 2. 2018 ;[citado 2024 set. 14 ]
Vancouver
South American Dark Matter Workshop, 2. 2018 ;[citado 2024 set. 14 ]
Artigo de periodico
Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. et al. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051103-1-051103-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051103. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051103-1-051103-8. doi:10.1103/PhysRevLett.121.051103
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
Artigo de periodico
Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station (2018)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
AGUILAR, M. et al. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 120, n. Ja 2018, p. 021101-1-021101-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.120.021101. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 120( Ja 2018), 021101-1-021101-8. doi:10.1103/PhysRevLett.120.021101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
Artigo de periodico
Indications for a high-rigidity break in the cosmic-ray diffusion coefficient (2017)
Génolini, Yoann; Serpico, Pasquale D.; Boudaud, Mathieu; Caroff, Sami; Poulin, Vivian; Derome, Laurent; Lavalle, Julien; Maurin, David; Poireau, Vincent; Rosier, Sylvie; Salati, Pierre; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
GÉNOLINI, Yoann et al. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, v. 119, n. 24, p. 241101-1-241101-6, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.241101. Acesso em: 14 set. 2024.
APA
Génolini, Y., Serpico, P. D., Boudaud, M., Caroff, S., Poulin, V., Derome, L., et al. (2017). Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, 119( 24), 241101-1-241101-6. doi:10.1103/PhysRevLett.119.241101
NLM
Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101
Vancouver
Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101
Trabalho de evento-anais periodico
What do Galactic electrons and positrons tell us about dark matter? (2017)
Boudaud, M.; Bueno, E. F.; Caroff, S.; Putze, A.; Genolini, Y.; Lavalle, J.; Poireau, V.; Poulin, V.; Rosier, S.; Salati, P.; Vecchi, Manuela
Source: Proceedings of Science. Conference titles: International Cosmic Ray Conference - ICRC. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, FÍSICA DE PARTÍCULAS
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ABNT
BOUDAUD, M. et al. What do Galactic electrons and positrons tell us about dark matter?. Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. Disponível em: https://doi.org/10.22323/1.301.0915. Acesso em: 14 set. 2024. , 2017
APA
Boudaud, M., Bueno, E. F., Caroff, S., Putze, A., Genolini, Y., Lavalle, J., et al. (2017). What do Galactic electrons and positrons tell us about dark matter? Proceedings of Science. Trieste: Scuola Internazionale Superiore di Studi Avanzati - SISSA. doi:10.22323/1.301.0915
NLM
Boudaud M, Bueno EF, Caroff S, Putze A, Genolini Y, Lavalle J, Poireau V, Poulin V, Rosier S, Salati P, Vecchi M. What do Galactic electrons and positrons tell us about dark matter? [Internet]. Proceedings of Science. 2017 ; 301 915-1-915-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.22323/1.301.0915
Vancouver
Boudaud M, Bueno EF, Caroff S, Putze A, Genolini Y, Lavalle J, Poireau V, Poulin V, Rosier S, Salati P, Vecchi M. What do Galactic electrons and positrons tell us about dark matter? [Internet]. Proceedings of Science. 2017 ; 301 915-1-915-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.22323/1.301.0915
Curadoria
South American Dark Matter Workshop (2017)
Betuzzo, Enrico (cur); Vecchi, Manuela (cur)
Unidades: IF, IFSC
Subjects: MATÉRIA ESCURA, FÍSICA TEÓRICA, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
South American Dark Matter Workshop. . São Paulo: International Centre for Theoretical Physics, ICTP, South American Institute for Fundamental Research, SAIFR. . Acesso em: 14 set. 2024. , 2017
APA
South American Dark Matter Workshop. (2017). South American Dark Matter Workshop. São Paulo: International Centre for Theoretical Physics, ICTP, South American Institute for Fundamental Research, SAIFR.
NLM
South American Dark Matter Workshop. 2017 ;[citado 2024 set. 14 ]
Vancouver
South American Dark Matter Workshop. 2017 ;[citado 2024 set. 14 ]
Artigo de periodico
Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station (2017)
Aguilar, M.; Bueno, E. F.; Lordello, V. D.; Mikuni, V. M.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. et al. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 119, n. 25, p. 251101-1-241101-8, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.251101. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2017). Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 119( 25), 251101-1-241101-8. doi:10.1103/PhysRevLett.119.251101
NLM
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
Vancouver
Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
Artigo de periodico
Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946 (2017)
Acero, F.; Dal Pino, Elisabete Maria de Gouveia; Falceta Gonçalves, Diego Antonio; Melioli, C.; Silva, Rodrigo Nemmen da; Vecchi, Manuela
Source: Astrophysical Journal. Unidades: EACH, IAG, IFSC
Subjects: FÍSICA DE ALTA ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ACERO, F. et al. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946. Astrophysical Journal, v. 840, n. 2, p. 74-1-74-14, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6d67. Acesso em: 14 set. 2024.
APA
Acero, F., Dal Pino, E. M. de G., Falceta Gonçalves, D. A., Melioli, C., Silva, R. N. da, & Vecchi, M. (2017). Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946. Astrophysical Journal, 840( 2), 74-1-74-14. doi:10.3847/1538-4357/aa6d67
NLM
Acero F, Dal Pino EM de G, Falceta Gonçalves DA, Melioli C, Silva RN da, Vecchi M. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946 [Internet]. Astrophysical Journal. 2017 ; 840( 2): 74-1-74-14.[citado 2024 set. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6d67
Vancouver
Acero F, Dal Pino EM de G, Falceta Gonçalves DA, Melioli C, Silva RN da, Vecchi M. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946 [Internet]. Astrophysical Journal. 2017 ; 840( 2): 74-1-74-14.[citado 2024 set. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6d67
Artigo de periodico
The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements (2017)
Boudaud, M.; Bueno, E. F.; Caroff, S.; Genolini, Y.; Poulin, V.; Poireau, V.; Putze, A.; Rosier, S.; Salati, P.; Vecchi, Manuela
Source: Astronomy and Astrophysics. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BOUDAUD, M. et al. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements. Astronomy and Astrophysics, v. 605, p. A17-1-A17-16, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201630321. Acesso em: 14 set. 2024.
APA
Boudaud, M., Bueno, E. F., Caroff, S., Genolini, Y., Poulin, V., Poireau, V., et al. (2017). The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements. Astronomy and Astrophysics, 605, A17-1-A17-16. doi:10.1051/0004-6361/201630321
NLM
Boudaud M, Bueno EF, Caroff S, Genolini Y, Poulin V, Poireau V, Putze A, Rosier S, Salati P, Vecchi M. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements [Internet]. Astronomy and Astrophysics. 2017 ; 605 A17-1-A17-16.[citado 2024 set. 14 ] Available from: https://doi.org/10.1051/0004-6361/201630321
Vancouver
Boudaud M, Bueno EF, Caroff S, Genolini Y, Poulin V, Poireau V, Putze A, Rosier S, Salati P, Vecchi M. The pinching method for galactic cosmic ray positrons: implications in the light of precision measurements [Internet]. Astronomy and Astrophysics. 2017 ; 605 A17-1-A17-16.[citado 2024 set. 14 ] Available from: https://doi.org/10.1051/0004-6361/201630321
Artigo de periodico
Optical and x-ray early follow-up of ANTARES neutrino alerts (2016)
Adrián-Martínez, S.; Vecchi, Manuela
Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ADRIÁN-MARTÍNEZ, S. e VECCHI, Manuela. Optical and x-ray early follow-up of ANTARES neutrino alerts. Journal of Cosmology and Astroparticle Physics, v. 2016, p. 062-1-062-25, 2016Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2016/02/062. Acesso em: 14 set. 2024.
APA
Adrián-Martínez, S., & Vecchi, M. (2016). Optical and x-ray early follow-up of ANTARES neutrino alerts. Journal of Cosmology and Astroparticle Physics, 2016, 062-1-062-25. doi:10.1088/1475-7516/2016/02/062
NLM
Adrián-Martínez S, Vecchi M. Optical and x-ray early follow-up of ANTARES neutrino alerts [Internet]. Journal of Cosmology and Astroparticle Physics. 2016 ; 2016 062-1-062-25.[citado 2024 set. 14 ] Available from: https://doi.org/10.1088/1475-7516/2016/02/062
Vancouver
Adrián-Martínez S, Vecchi M. Optical and x-ray early follow-up of ANTARES neutrino alerts [Internet]. Journal of Cosmology and Astroparticle Physics. 2016 ; 2016 062-1-062-25.[citado 2024 set. 14 ] Available from: https://doi.org/10.1088/1475-7516/2016/02/062
Artigo de periodico
Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station (2016)
Aguilar, M.; Bueno, E. F.; Vecchi, Manuela
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, v. 117, n. 9, p. 091103-1-091103-10, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.091103. Acesso em: 14 set. 2024.
APA
Aguilar, M., Bueno, E. F., & Vecchi, M. (2016). Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, 117( 9), 091103-1-091103-10. doi:10.1103/PhysRevLett.117.091103
NLM
Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103
Vancouver
Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103

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