Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/25851
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kang, D. | en_US |
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 | 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 | Feng, Z. | 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 | Huber, D. | en_US |
dc.contributor.author | Huege, T. | en_US |
dc.contributor.author | Kampert, K. H. | 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 | Palmieri, N. | en_US |
dc.contributor.author | Petcu, M. | 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. | 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 | 2020-06-01T13:35:18Z | - |
dc.date.available | 2020-06-01T13:35:18Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 1742-6588 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/25851 | - |
dc.description.abstract | Using data measured by the KASCADE-Grande air shower array, an upper limit to the flux of ultra-high energy gamma-rays in the primary cosmic-ray flux is determined. KASCADE-Grande measures the electromagnetic and muonic components for individual air showers in the energy range from 10 PeV up to 1 EeV. The analysis is performed by selecting air showers with low muon contents. A preliminary result on the 90% C.L. upper limit to the relative intensity of gamma-ray with respect to cosmic ray primaries is presented and compared with limits reported by other measurements. | en_US |
dc.language.iso | eng | en_US |
dc.title | A limit on the diffuse gamma-rays measured with KASCADE-Grande | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1088/1742-6596/632/1/012013 | en_US |
dc.identifier.scopus | 2-s2.0-84940702450 | en_US |
dc.identifier.isi | 000362286200013 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/1742-6596/632/1/012013 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 632 | en_US |
dc.relation.issue | 1 | en |
dc.relation.firstpage | 012013 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.ispartofbook | 24th European Cosmic Ray Symposium (ECRS) | en_US |
dc.relation.conferencename | 24th European Cosmic Ray Symposium (ECRS) | en_US |
dc.relation.conferenceplace | Kiel, Germany | en_US |
dc.relation.conferencedate | 1–5 September, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF PHYSICS. CONFERENCE SERIES | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015JPhCS.632a2013K | 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.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
crisitem.journal.journalissn | 1742-6588 | - |
crisitem.journal.ance | E187130 | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0003-0866-6379 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Kang_2015_J._Phys.__Conf._Ser._632_012013.pdf | Pdf editoriale | 1.43 MB | Adobe PDF | View/Open |
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