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Measurement of the cosmic-ray energy spectrum above 2.5 x 10¹⁸ eV using the Pierre Auger Observatory

Aab, A.
Abreu, P.
Aglietta, M.
Albury, J.M.
Allekotte, I.
Almela, A.
Castillo, J.A.
Alvarez-Muniz, J.
Batista, R.A.
Anastasi, G.A.
Anchordoqui, L.
Andrada, B.
Andringa, S.
Aramo, C.
Ferreira, P.R.A.
Asorey, H.
Assis, P.
Avila, G.
Badescu, A.M.
Bakalova, A.
et al.

January 2020

We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...

Evidence for a high-energy cosmic-ray spectrum cutoff

Sokolsky, Pierre
Baltrusaitis, R. M.

April 1985

Journal ArticleWe report a measurement of the ultrahigh-energy cosmic-ray spectrum using an atmosphe...

Energy spectrum of cascades generated by muons in Baksan underground scintillation telescope

Stenkin, Y. V.
Achkasov, V. M.
Bakatanov, V. N.
Chudakov, A. E.
Semenov, A. M.
Novoseltseva, M. V.
Novoseltsev, Y. F.

August 1985

Spectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle o...

Unmasking the tail of the cosmic ray spectrum

Anchordoqui, L A
Dova, M T
McCauley, T P
Reucroft, S
Swain, J D

January 2000

A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...

Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory

Pierre Auger collaboration (463 authors)
Abreu, Pedro
Andringa, Sofia
Assis, Pedro
Blanco, Alberto
Brogueira, Pedro
Cazon, Lorenzo
Conceição, Ruben
Diogo, Francisco
Espadanal, Joao
Lopes, Luis
Pimenta, Mário
Santos, Eva
Sarmento, Raul
Tomé, Bernardo

February 2019

A measurement of the cosmic-ray spectrum for energies exceeding 4×10(18) eV is presented, which is b...

Measurement of the cosmic-ray energy spectrum above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

January 2020

International audienceWe report a measurement of the energy spectrum of cosmic rays for energies abo...

Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

January 2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using...

Measurement of the cosmic-ray energy spectrum above 2.5 x 10¹⁸ eV using the Pierre Auger Observatory

Aab, A.
Abreu, P.
Aglietta, M.
Albury, J.M.
Allekotte, I.
Almela, A.
Castillo, J.A.
Alvarez-Muniz, J.
Batista, R.A.
Anastasi, G.A.
Anchordoqui, L.
Andrada, B.
Andringa, S.
Aramo, C.
Ferreira, P.R.A.
Asorey, H.
Assis, P.
Avila, G.
Badescu, A.M.
Bakalova, A.
et al.

January 2020

We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...

Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory

Pierre Auger collaboration (463 authors)
Abreu, Pedro
Andringa, Sofia
Assis, Pedro
Blanco, Alberto
Brogueira, Pedro
Cazon, Lorenzo
Conceição, Ruben
Diogo, Francisco
Espadanal, Joao
Lopes, Luis
Pimenta, Mário
Santos, Eva
Sarmento, Raul
Tomé, Bernardo

February 2019

A measurement of the cosmic-ray spectrum for energies exceeding 4×10(18) eV is presented, which is b...

Measurement of the cosmic-ray energy spectrum above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

January 2020

International audienceWe report a measurement of the energy spectrum of cosmic rays for energies abo...

Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

January 2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using...

Measurement of the cosmic-ray energy spectrum above 2.5 x 10¹⁸ eV using the Pierre Auger Observatory

Aab, A.
Abreu, P.
Aglietta, M.
Albury, J.M.
Allekotte, I.
Almela, A.
Castillo, J.A.
Alvarez-Muniz, J.
Batista, R.A.
Anastasi, G.A.
Anchordoqui, L.
Andrada, B.
Andringa, S.
Aramo, C.
Ferreira, P.R.A.
Asorey, H.
Assis, P.
Avila, G.
Badescu, A.M.
Bakalova, A.
et al.

January 2020

We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based ...