Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26646
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Porquet, D. | en_US |
dc.contributor.author | Reeves, J. | en_US |
dc.contributor.author | Lobban, A. | en_US |
dc.contributor.author | BRAITO, Valentina | en_US |
dc.contributor.author | NARDINI, EMANUELE | en_US |
dc.contributor.author | Grosso, N. | en_US |
dc.contributor.author | Matt, G. | en_US |
dc.contributor.author | Marinucci, A. | en_US |
dc.contributor.author | TORTOSA, ALESSIA | en_US |
dc.contributor.author | Ursino, F. | en_US |
dc.date.accessioned | 2020-07-27T09:52:21Z | - |
dc.date.available | 2020-07-27T09:52:21Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26646 | - |
dc.description.abstract | The physical characteristics of the matter around supermassive black hole (SMBH) are currently determined thanks to X-ray observations. However, the origins of the main X-ray spectral components such as the soft X-ray excess, the FeK line complex and the hard X-ray excess are still hotly debated. This is difficult to investigate in AGN which show a significant warm absorber that severely distort the continuum. Therefore, AGN which show no (or very weak) warm absorption on the line-of-sight, so-called "bare AGN'' are the best targets to probe the processes at work very close to the SMBH. We will present the first results from an extensive observation campaign (XMM-Newton Large Program, Chandra/HETG, NuSTAR) of Ark120 that is the brightest and cleanest bare AGN known so far. We will focus on the analysis of the deep RGS spectrum, as well as on the X-ray broad band spectrum. | en_US |
dc.language.iso | eng | en_US |
dc.title | A deep X-ray view of the bare nucleus Seyfert Ark120: unveiling the core of AGN | en_US |
dc.type | Multimedia | - |
dc.identifier.url | https://www.cosmos.esa.int/documents/332006/1402684/DPorquet_t.pdf | en_US |
dc.identifier.url | https://www.cosmos.esa.int/web/xmm-newton/2017-symposium | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 180 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.international | sì | en_US |
dc.relation.ispartofbook | The X-ray Universe 2017 | en_US |
dc.relation.conferencename | The X-ray Universe 2017 | en_US |
dc.relation.conferenceplace | Rome, Italy | en_US |
dc.relation.conferencedate | 6-9 June, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 298 Altro | - |
dc.identifier.adsbibcode | 2017xru..conf..180P | 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.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Multimedia | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0002-2629-4989 | - |
crisitem.author.orcid | 0000-0001-9226-8992 | - |
crisitem.author.orcid | 0000-0003-3450-6483 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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DPorquet_t.pdf | Talk | 899.54 kB | Adobe PDF | View/Open |
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