Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23872| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Pierre Auger Collaboration | - |
| dc.contributor.author | AGLIETTA, MARCO | - |
| dc.contributor.author | CASTELLINA, ANTONELLA | - |
| dc.contributor.author | GORGI, Alessio | - |
| dc.contributor.author | MESSINA, Sergio | - |
| dc.contributor.author | RIGGI, Simone | - |
| dc.contributor.author | SEGRETO, ALBERTO | - |
| dc.contributor.author | Zuccarello, Francesca | - |
| dc.date.accessioned | 2020-04-06T11:16:25Z | - |
| dc.date.available | 2020-04-06T11:16:25Z | - |
| dc.date.issued | 2015 | - |
| dc.identifier.issn | 1475-7516 | - |
| dc.identifier.uri | http://hdl.handle.net/20.500.12386/23872 | - |
| dc.description.abstract | A measurement of the cosmic-ray spectrum for energies exceeding 4×10<SUP>18</SUP> eV is presented, which is based on the analysis of showers with zenith angles greater than 60° detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.3×10<SUP>18</SUP> eV, the ``ankle'', the flux can be described by a power law E<SUP>-γ</SUP> with index γ=2.70 ± 0.02 (stat) ± 0.1 (sys) followed by a smooth suppression region. For the energy (E<SUB>s</SUB>) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find E<SUB>s</SUB>=(5.12±0.25 (stat)<SUP>+1.0</SUP><SUB>-1.2</SUB> (sys))×10<SUP>19</SUP> eV. | - |
| dc.language.iso | eng | - |
| dc.title | Measurement of the cosmic ray spectrum above 4 × 10<SUP>18</SUP> eV using inclined events detected with the Pierre Auger Observatory | - |
| dc.type | Article | - |
| dc.identifier.doi | 10.1088/1475-7516/2015/08/049 | en_US |
| dc.identifier.scopus | 2-s2.0-84941649751 | en_US |
| dc.identifier.isi | 000365046600049 | en_US |
| dc.identifier.url | https://iopscience.iop.org/article/10.1088/1475-7516/2015/08/049 | - |
| dc.relation.medium | STAMPA | - |
| dc.relation.volume | 2015 | - |
| dc.relation.issue | 8 | - |
| dc.relation.firstpage | 049 | - |
| dc.relation.lastpage | 049 | - |
| dc.type.referee | REF_1 | - |
| dc.description.international | sì | - |
| dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | - |
| dc.relation.journal | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | - |
| dc.type.miur | 262 Articolo in rivista | - |
| dc.identifier.adsbibcode | 2015JCAP...08..049P | - |
| dc.description.apc | no | - |
| dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | - |
| item.openairetype | Article | - |
| item.fulltext | With Fulltext | - |
| item.grantfulltext | open | - |
| item.languageiso639-1 | en | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.cerifentitytype | Publications | - |
| crisitem.journal.journalissn | 1475-7516 | - |
| crisitem.journal.ance | E184073 | - |
| crisitem.author.dept | O.A. Torino | - |
| crisitem.author.dept | O.A. Torino | - |
| crisitem.author.dept | O.A. Torino | - |
| crisitem.author.dept | O.A. Catania | - |
| crisitem.author.dept | IASF Palermo | - |
| crisitem.author.dept | O.A. Catania | - |
| crisitem.author.orcid | 0000-0001-8354-5388 | - |
| crisitem.author.orcid | 0000-0002-0045-2467 | - |
| crisitem.author.orcid | 0000-0002-8085-2304 | - |
| crisitem.author.orcid | 0000-0001-6368-8330 | - |
| crisitem.author.orcid | 0000-0001-7341-6603 | - |
| crisitem.author.orcid | 0000-0003-1853-2550 | - |
| Appears in Collections: | 1.01 Articoli in rivista | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 1503.07786-doi10.10881475-7516201508049.pdf | postprint | 814.94 kB | Adobe PDF | View/Open |
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