Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28422
DC Field | Value | Language |
---|---|---|
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 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Vercellone_AIPC_2018_1792_id.030001.pdf | Pdf editoriale | 2.19 MB | Adobe PDF | View/Open |
Page view(s)
42
checked on Apr 25, 2024
Download(s)
14
checked on Apr 25, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.