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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/31212
DC FieldValueLanguage
dc.contributor.authorMALIZIA, ANGELAen_US
dc.contributor.authorSergey Sazonoven_US
dc.contributor.authorBASSANI, LOREDANAen_US
dc.contributor.authorPIAN, Elenaen_US
dc.contributor.authorVolker Beckmannen_US
dc.contributor.authorMOLINA, MANUELAen_US
dc.contributor.authorIlya Mereminskiyen_US
dc.contributor.authorGuillaume Belangeren_US
dc.date.accessioned2021-12-09T15:54:45Z-
dc.date.available2021-12-09T15:54:45Z-
dc.date.issued2020en_US
dc.identifier.issn1387-6473en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/31212-
dc.description.abstractAGN are among the most energetic phenomena in the Universe and in the last two decades INTEGRAL's contribution in their study has had a significant impact. Thanks to the INTEGRAL extragalactic sky surveys, all classes of soft X-ray detected (in the 2-10 keV band) AGN have been observed at higher energies as well. Up to now, around 450 AGN have been catalogued and a conspicuous part of them are either objects observed at high-energies for the first time or newly discovered AGN. The high-energy domain (20-200 keV) represents an important window for spectral studies of AGN and it is also the most appropriate for AGN population studies, since it is almost unbiased against obscuration and therefore free of the limitations which affect surveys at other frequencies. Over the years, INTEGRAL data have allowed to characterise AGN spectra at high energies, to investigate their absorption properties, to test the AGN unification scheme and to perform population studies. In this review the main results are reported and INTEGRAL's contribution to AGN science is highlighted for each class of AGN. Finally, new perspectives are provided, connecting INTEGRAL's science with that at other wavelengths and in particular to the GeV/TeV regime which is still poorly explored.en_US
dc.language.isoengen_US
dc.titleINTEGRAL view of AGNen_US
dc.typeArticle-
dc.identifier.doi10.1016/j.newar.2020.101545en_US
dc.identifier.scopus2-s2.0-85094580936en_US
dc.identifier.isiWOS:000594177100002en_US
dc.identifier.urlhttps://www.sciencedirect.com/science/article/pii/S1387647320300221?via%3Dihuben_US
dc.identifier.urlhttp://arxiv.org/abs/2009.03232v1en_US
dc.relation.mediumSTAMPAen_US
dc.relation.volume90en_US
dc.relation.firstpage101545en_US
dc.relation.lastpage101575en_US
dc.relation.numberofpages30en_US
dc.type.refereeREF_1en_US
dc.description.internationalsìen_US
dc.contributor.countryFRAen_US
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.relation.journalNEW ASTRONOMY REVIEWSen_US
dc.type.miur262 Articolo in rivista-
dc.identifier.adsbibcode2020NewAR..9001545Men_US
dc.description.apcnoen_US
dc.description.oa1 – prodotto con file in versione Open Access (allegare il file al passo  5-Carica)en_US
item.cerifentitytypePublications-
item.fulltextWith Fulltext-
item.openairetypeArticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.languageiso639-1en-
item.grantfulltextopen-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptIASF Milano-
crisitem.author.orcid0000-0002-6558-1163-
crisitem.author.orcid0000-0003-4858-6963-
crisitem.author.orcid0000-0001-8646-4858-
crisitem.author.orcid0000-0003-0681-9984-
crisitem.journal.journalissn1387-6473-
crisitem.journal.anceE117454-
Appears in Collections:1.01 Articoli in rivista
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2009.03232-2.pdfpreprint1.07 MBAdobe PDFView/Open
1-s2.0-S1387647320300221-compr.pdf[Administrators only]1.41 MBAdobe PDF
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