Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28422
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | VERCELLONE, STEFANO | en_US |
dc.date.accessioned | 2020-11-18T15:28:45Z | - |
dc.date.available | 2020-11-18T15:28:45Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.isbn | 978-0-7354-1456-3 | en_US |
dc.identifier.issn | 0094-243X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28422 | - |
dc.description.abstract | The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, open to the scientific community, to investigate the very high-energy emission from a large variety of celestial sources in the energy range 20 GeV - 300 TeV. The full array, distributed over two sites, one in the northern and one in the southern hemisphere, will provide whole-sky coverage and will improve by about one order of magnitude the sensitivity with respect to the current major arrays. CTA will investigate a much higher number of already known classes of sources, going to much larger distances in the Universe, performing population studies, accurate variability and spatially-resolved studies. Moreover, new light will be shed on possible new classes of high-energy sources, such as GRBs, cluster of Galaxies, Galactic binaries, and on fundamental physics. By pushing the high-energy limit to E > 100 TeV it will allow a thorough exploration of the cut-off regime of the cosmic accelerators. We review the main CTA Key Science Projects, which will focus on major scientific cases, a clear advance beyond the current state of the art, and we discuss the production of legacy data-sets of high value to a wider community. | en_US |
dc.language.iso | eng | en_US |
dc.title | The key science projects of the Cherenkov telescope array | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1063/1.4968902 | en_US |
dc.identifier.scopus | 2-s2.0-85010966180 | en_US |
dc.identifier.isi | 000399207800017 | en_US |
dc.identifier.url | https://aip.scitation.org/doi/abs/10.1063/1.4968902 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 1792 | en_US |
dc.relation.issue | 1 | en |
dc.relation.firstpage | 030001-01 | en_US |
dc.relation.lastpage | 030001-12 | en_US |
dc.relation.numberofpages | 12 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.alleditors | Aharonian, Felix A.; Hofmann, Werner; Rieger, Frank M. | en_US |
dc.relation.ispartofbook | HIGH ENERGY GAMMA-RAY ASTRONOMY: 6th International Meeting on High Energy Gamma-Ray Astronomy | en_US |
dc.type.invited | sì | en_US |
dc.relation.conferencename | HIGH ENERGY GAMMA-RAY ASTRONOMY: 6th International Meeting on High Energy Gamma-Ray Astronomy | en_US |
dc.relation.conferenceplace | Heidelberg, Germany | en_US |
dc.relation.conferencedate | 11–15 July, 2016 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | AIP CONFERENCE PROCEEDINGS | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2017AIPC.1792c0001V | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0003-1163-1396 | - |
crisitem.journal.journalissn | 0094-243X | - |
crisitem.journal.ance | E211233 | - |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
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Vercellone_AIPC_2018_1792_id.030001.pdf | Pdf editoriale | 2.19 MB | Adobe PDF | Visualizza/apri |
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