Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24337
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Zaino, Alessandra | en_US |
dc.contributor.author | SEVERGNINI, Paola | en_US |
dc.contributor.author | Vignali, C. | en_US |
dc.contributor.author | DELLA CECA, Roberto | en_US |
dc.contributor.author | Ballo, L. | en_US |
dc.date.accessioned | 2020-04-29T15:23:56Z | - |
dc.date.available | 2020-04-29T15:23:56Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24337 | - |
dc.description.abstract | An efficient diagnostic method to find local (z<0.1) Compton-thick AGN consists in selecting sources characterized by hard X- ray colors and low hard X-ray over mid-IR flux ratio. This has been done efficiently in the past using 2XMM and IRAS data (Severgnini et al. 2012). In this talk I will present my thesis work in which I tested this technique using the latest 3XMM and WISE data for the sample presented by Severgnini et al. I will also briefly discuss the X-ray spectral properties of all of those sources showing flux and/or spectral variability in the XMM-Newton observations. | en_US |
dc.language.iso | eng | en_US |
dc.title | AGN Diagnostic Plot In The WISE And 3XMM Era: The Role Of Variability | en_US |
dc.type | Multimedia | - |
dc.identifier.doi | 10.5281/zenodo.163800 | en_US |
dc.identifier.url | https://zenodo.org/record/163800#.Xp8s5K3W4ht | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 43 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.ispartofbook | Active Galactic Nuclei 12: A Multi-Messenger Perspective (AGN12) | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Active Galactic Nuclei 12: A Multi-Messenger Perspective (AGN12) | en_US |
dc.relation.conferenceplace | Napoli, Italy | en_US |
dc.relation.conferencedate | 26-29 September, 2016 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 298 Altro | - |
dc.identifier.adsbibcode | 2016agnt.confE..43Z | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Multimedia | - |
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.orcid | 0000-0001-5619-5896 | - |
crisitem.author.orcid | 0000-0001-7551-2252 | - |
Appears in Collections: | 4.09 Prodotti multimediali |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
agn12_zaino_talk.pdf | 3.88 MB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.