

You have already added 0 works in your ORCID record related to the merged Research product.
You have already added 0 works in your ORCID record related to the merged Research product.
<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>
Measurement of the energy spectrum of cosmic rays above 1018 eV using the Pierre Auger Observatory

arXiv: 1002.1975
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 10^18 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^-gamma with index gamma=3.3 below the ankle which is measured at log10(E/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.
Accepted for publication in Physics Letters B
- University of Chicago United States
- University of Oxford United Kingdom
- University of Nebraska System United States
- The Ohio State University United States
- University of Nebraska System United States
Photon fraction, System, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, UPPER LIMIT, PHOTON FRACTION, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, info:eu-repo/classification/ddc/530, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics, ddc:530, Pierre Auger Observatory, 520, ELECTRONS, SIMULATION, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Cosmic rays; Energy spectrum; Pierre Auger Observatory, Simulation, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Showers, 539.1, energy spectrum, FOS: Physical sciences, Electrons, SURFACE DETECTOR, 530, cosmic rays, SHOWERS, Cosmic rays, Array., Surface detector, Upper limit, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Física, 2207 Física Atómica y Nuclear, ARRAY, Energy spectrum, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], SYSTEM
Photon fraction, System, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, UPPER LIMIT, PHOTON FRACTION, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, info:eu-repo/classification/ddc/530, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics, ddc:530, Pierre Auger Observatory, 520, ELECTRONS, SIMULATION, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Cosmic rays; Energy spectrum; Pierre Auger Observatory, Simulation, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Showers, 539.1, energy spectrum, FOS: Physical sciences, Electrons, SURFACE DETECTOR, 530, cosmic rays, SHOWERS, Cosmic rays, Array., Surface detector, Upper limit, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Física, 2207 Física Atómica y Nuclear, ARRAY, Energy spectrum, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], SYSTEM
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).372 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 1% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 1% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 0.1% visibility views 160 download downloads 575 - 160views575downloads
Data source Views Downloads Servicio de Difusión de la Creación Intelectual 6 222 DIGITAL.CSIC 12 29 Full-text Institutional Repository of the Ruđer Bošković Institute 142 324


