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Description
  • We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using the Pierre Auger Observatory. Based on fluorescence observations in coincidence with at least one surface detector we derive a spectrum for energies above 1018 eV. We also update the previously published energy spectrum obtained with the surface detector array. The two spectra are combined addressing the systematic uncertainties and, in particular, the influence of the energy resolution on the spectral shape. The spectrum can be described by a broken power law E-gama with index gama=3.3 below the ankle which is measured at log10(Eankle/eV) = 18.6. Above the ankle the spectrum is described by a power law with index 2.6 followed by a flux suppression, above about log10(E/eV) = 19.5, detected with high statistical significance.
  • We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using the Pierre Auger Observatory. Based on fluorescence observations in coincidence with at least one surface detector we derive a spectrum for energies above 1018 eV. We also update the previously published energy spectrum obtained with the surface detector array. The two spectra are combined addressing the systematic uncertainties and, in particular, the influence of the energy resolution on the spectral shape. The spectrum can be described by a broken power law E-gama with index gama=3.3 below the ankle which is measured at log10(Eankle/eV) = 18.6. Above the ankle the spectrum is described by a power law with index 2.6 followed by a flux suppression, above about log10(E/eV) = 19.5, detected with high statistical significance. (en)
Title
  • Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory
  • Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory (en)
skos:prefLabel
  • Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory
  • Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory (en)
skos:notation
  • RIV/61989592:15310/10:10215723!RIV12-MSM-15310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(1M06002), P(KJB100100904), P(KJB300100801), P(LA08016), P(LC527), Z(AV0Z10100502), Z(AV0Z10100522), Z(MSM0021620859)
http://linked.open...iv/cisloPeriodika
  • 4-5
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 270048
http://linked.open...ai/riv/idVysledku
  • RIV/61989592:15310/10:10215723
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Observatory; Auger; Pierre; using; 10^18; above; rays; cosmic; spectrum; energy; Measurement (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • NL - Nizozemsko
http://linked.open...ontrolniKodProRIV
  • [4E501CC1A2CB]
http://linked.open...i/riv/nazevZdroje
  • Physics Letters. Section B: Nuclear, Elementary Particle and High-Energy Physics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 685
http://linked.open...iv/tvurceVysledku
  • Abreu, P.
  • Aglietta, M.
  • Hrabovský, Miroslav
  • Rössler, Tomáš
  • Halenka, Viktor
  • Abraham, J.
http://linked.open...ain/vavai/riv/wos
  • 000275640600003
http://linked.open...n/vavai/riv/zamer
issn
  • 0370-2693
number of pages
http://localhost/t...ganizacniJednotka
  • 15310
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