Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/24139
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | BALLO, Lucia | en_US |
dc.contributor.author | SEVERGNINI, Paola | en_US |
dc.contributor.author | MORETTI, Alberto | en_US |
dc.contributor.author | DELLA CECA, Roberto | en_US |
dc.contributor.author | ANDREON, Stefano | en_US |
dc.contributor.author | BRAITO, Valentina | en_US |
dc.contributor.author | CACCIANIGA, Alessandro | en_US |
dc.contributor.author | CAMPANA, Sergio | en_US |
dc.contributor.author | VIGNALI, CRISTIAN | en_US |
dc.date.accessioned | 2020-04-21T08:28:48Z | - |
dc.date.available | 2020-04-21T08:28:48Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24139 | - |
dc.description.abstract | One of the key ingredients of the Unified Model of Active Galactic Nuclei (AGN) is the presence of a torus-like optically thick medium composed by dust and gas around the putative supermassive black hole. However, the structure, size and composition of this circumnuclear medium are still matter of debate. To this end, the search for column density variations through X-ray monitoring on different timescales (months, weeks and few days) is fundamental to constrain size, kinematics and location of the X-ray absorber(s). Here we describe our project of mining the Swift-XRT archive to assemble a sample of AGN with extreme column density variability and determining the physical properties of the X-ray absorber(s). We also present the results obtained from a daily-weekly Swift-XRT follow-up monitoring recently performed on one of the most interesting new candidates for variability discovered so far, Mrk 915. | en_US |
dc.language.iso | eng | en_US |
dc.title | Mining the XRT archive to probe the X-ray absorber structure in the AGN population | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.22323/1.233.0122 | en_US |
dc.identifier.url | https://pos.sissa.it/233/122 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 233 | en_US |
dc.relation.firstpage | 122 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 9 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.ispartofbook | Swift: 10 Years of Discovery (SWIFT 10) | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Swift: 10 Years of Discovery (SWIFT 10) | en_US |
dc.relation.conferenceplace | Roma | en_US |
dc.relation.conferencedate | 2-5 December 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015arXiv150502593B | 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.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0001-5619-5896 | - |
crisitem.author.orcid | 0000-0002-9770-0315 | - |
crisitem.author.orcid | 0000-0001-7551-2252 | - |
crisitem.author.orcid | 0000-0002-2041-8784 | - |
crisitem.author.orcid | 0000-0002-2629-4989 | - |
crisitem.author.orcid | 0000-0002-2339-8264 | - |
crisitem.author.orcid | 0000-0001-6278-1576 | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
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