About: Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

Facets (new session)
Description
Metadata
Settings
- owl:sameAs
- Inference Rule:

About: Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory Goto Sponge NotDistinct Permalink

An Entity of Type : http://linked.opendata.cz/ontology/domain/vavai/Vysledek, within Data Space : linked.opendata.cz associated with source document(s)

Attributes	Values
rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
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	P Z
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	2012
http://linked.open...aciTvurceVysledku	Rössler, Tomáš Halenka, Viktor Hrabovský, Miroslav
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Univerzita Palackého v Olomouci / Přírodovědecká fakulta
http://linked.open...dnocenehoVysledku	270048
http://linked.open...ai/riv/idVysledku	RIV/61989592:15310/10:10215723
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	Observatory; Auger; Pierre; using; 10^18; above; rays; cosmic; spectrum; energy; Measurement (en)
http://linked.open.../riv/klicoveSlovo	using energy rays Measurement Auger Observatory 10^18 above spectrum Pierre cosmic
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	BH
http://linked.open...ichTvurcuVysledku	3 (xsd:int)
http://linked.open...cetTvurcuVysledku	521 (xsd:int)
http://linked.open...vavai/riv/projekt	Optical structures, detection systems and relevant technologies for low photon number applications Study of parameters of atmospheric showers sensitive to mass composition of cosmic rays The origin of the highest-energy cosmic rays observed by the Auger experiment Participation in the project of the Pierre Auger Observatory Center for Particle Physics
http://linked.open...UplatneniVysledku	2010
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	Jevy fyziky elementárních částic přesahující standardní model Wave and Corpuscular Light Propagation, Optical Materials and Technology Výzkum vlastností jader a subjaderných částic a jejich interakcí
issn	0370-2693
number of pages	8 (xsd:int)
http://localhost/t...ganizacniJednotka	15310
is http://linked.open...avai/riv/vysledek of	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

Faceted Search & Find service v1.16.118 as of Jun 21 2024

Alternative Linked Data Documents: ODE Content Formats:

RDF

ODATA

Microdata

About

OpenLink Virtuoso version 07.20.3240 as of Jun 21 2024, on Linux (x86_64-pc-linux-gnu), Single-Server Edition (126 GB total memory, 77 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software