Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30176
DC Field | Value | Language |
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dc.contributor.author | Apel, W. D. | en_US |
dc.contributor.author | Arteaga-Velázquez, J. C. | en_US |
dc.contributor.author | Bekk, K. | en_US |
dc.contributor.author | Bertaina, M. | en_US |
dc.contributor.author | Blümer, J. | en_US |
dc.contributor.author | Bonino, R. | en_US |
dc.contributor.author | Bozdog, H. | en_US |
dc.contributor.author | Brancus, I. M. | en_US |
dc.contributor.author | Cantoni, E. | en_US |
dc.contributor.author | Chiavassa, A. | en_US |
dc.contributor.author | Cossavella, F. | en_US |
dc.contributor.author | Daumiller, K. | en_US |
dc.contributor.author | de Souza, V. | en_US |
dc.contributor.author | Di Pierro, F. | en_US |
dc.contributor.author | Doll, P. | en_US |
dc.contributor.author | Engel, R. | en_US |
dc.contributor.author | Fuhrmann, D. | en_US |
dc.contributor.author | Gherghel-Lascu, A. | en_US |
dc.contributor.author | Gils, H. J. | en_US |
dc.contributor.author | Glasstetter, R. | en_US |
dc.contributor.author | Grupen, C. | en_US |
dc.contributor.author | Haungs, A. | en_US |
dc.contributor.author | Heck, D. | en_US |
dc.contributor.author | Hörandel, J. R. | en_US |
dc.contributor.author | Huege, T. | en_US |
dc.contributor.author | Kampert, K. -H. | en_US |
dc.contributor.author | Kang, D. | en_US |
dc.contributor.author | Klages, H. O. | en_US |
dc.contributor.author | Link, K. | en_US |
dc.contributor.author | Łuczak, P. | en_US |
dc.contributor.author | Mathes, H. J. | en_US |
dc.contributor.author | Mayer, H. J. | en_US |
dc.contributor.author | Milke, J. | en_US |
dc.contributor.author | Mitrica, B. | en_US |
dc.contributor.author | Morello, C. | en_US |
dc.contributor.author | Oehlschläger, J. | en_US |
dc.contributor.author | Ostapchenko, S. | en_US |
dc.contributor.author | Pierog, T. | en_US |
dc.contributor.author | Rebel, H. | en_US |
dc.contributor.author | Roth, M. | en_US |
dc.contributor.author | Schieler, H. | en_US |
dc.contributor.author | Schoo, S. | en_US |
dc.contributor.author | Schröder, F. G. | en_US |
dc.contributor.author | Sima, O. | en_US |
dc.contributor.author | Toma, G. | en_US |
dc.contributor.author | TRINCHERO, GIAN CARLO | en_US |
dc.contributor.author | Ulrich, H. | en_US |
dc.contributor.author | Weindl, A. | en_US |
dc.contributor.author | Wochele, J. | en_US |
dc.contributor.author | Zabierowski, J. | en_US |
dc.date.accessioned | 2021-02-02T16:12:34Z | - |
dc.date.available | 2021-02-02T16:12:34Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30176 | - |
dc.description.abstract | We present the results of the search for large-scale anisotropies in the arrival directions of cosmic rays performed with the KASCADE-Grande experiment at energies higher than {10}<SUP>15</SUP> eV. To eliminate spurious anisotropies due to atmospheric or instrumental effects we apply the east-west method. We show, using the solar time distribution of the number of counts, that this technique allow us to remove correctly the count variations not associated to real anisotropies. By applying the east-west method we obtain the distribution of number of counts in intervals of 20 minutes of sidereal time. This distribution is then analyzed by searching for a dipole component; the significance of the amplitude of the first harmonic is 3.5σ, therefore, we derive its upper limit. The phase of the first harmonic is determined with an error of a few hours and is in agreement with the measurements obtained in the 10<SUP>14</SUP> < E < 2 × 10<SUP>15</SUP> eV energy range by the EAS-TOP, IceCube, and IceTop experiments. This supports the hypothesis of a change of the phase of the first harmonic at energies greater than ∼2 × 10<SUP>14</SUP> eV. | en_US |
dc.language.iso | eng | en_US |
dc.title | Search for Large-scale Anisotropy in the Arrival Direction of Cosmic Rays with KASCADE-Grande | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aaf1ca | en_US |
dc.identifier.scopus | 2-s2.0-85060217428 | en_US |
dc.identifier.isi | 000455820100037 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/aaf1ca | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 870 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 91 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019ApJ...870...91A | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0003-0866-6379 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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APJ_Anisotropy.pdf | Pdf editoriale | 417.39 kB | Adobe PDF | View/Open |
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