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http://hdl.handle.net/2307/285| Bed DC | Qiimo | Luqad |
|---|---|---|
| dc.contributor.author | Bianchi, Stefano | - |
| dc.contributor.author | Guainazzi, Matteo | - |
| dc.contributor.author | Matt, Giorgio | - |
| dc.contributor.author | Bonilla, N. Fonseca | - |
| dc.contributor.author | Ponti, Gabriele | - |
| dc.date.accessioned | 2010-07-09T09:31:56Z | - |
| dc.date.available | 2010-07-09T09:31:56Z | - |
| dc.date.issued | 2009-02 | - |
| dc.identifier.issn | 0004-6361 | - |
| dc.identifier.uri | http://hdl.handle.net/2307/285 | - |
| dc.description.abstract | Aims. We present CAIXA, a Catalogue of AGN In the XMM-Newton Archive.It consists of all the radio-quiet X-ray unobscured (N-H < 2 x 10(22)cm(-2)) active galactic nuclei (AGN) observed by XMM-Newton in targetedobservations, whose data are public as of March 2007. With its 156sources, this is the largest catalogue of high signal-to-noise X-rayspectra of AGN.Methods. All the EPIC pn spectra of the sources in CAIXA were extractedhomogeneously, and a baseline model was applied in order to derivetheir basic X-ray properties. These data are complemented bymultiwavelength data found in the literature: black hole masses, fullwidth half maximum (FWHM) of H beta, radio and optical fluxes.Results. Here we describe our homogeneous spectral analysis of theX-ray data in CAIXA and present all the results on the parametersadopted in our best-fit models. | en |
| dc.language.iso | en | en |
| dc.publisher | EDP Sciences | en |
| dc.relation.ispartof | Astronomy & Astrophysics | en |
| dc.subject | ACTIVE GALACTIC NUCLEI | en |
| dc.subject | BLACK-HOLE MASSES | en |
| dc.subject | LINE SEYFERT-1 GALAXIES | en |
| dc.subject | X-RAY VARIABILITY | en |
| dc.subject | NARROW-LINE | en |
| dc.subject | RADIO-SOURCES | en |
| dc.subject | IRON-LINE | en |
| dc.subject | ACCRETION | en |
| dc.subject | HOST GALAXIES | en |
| dc.subject | REGION SIZES | en |
| dc.title | CAIXA: a catalogue of AGN in the XMM-Newton archive I. Spectral analysis | en |
| dc.type | Article | en |
| dc.subject.miur | Settori Disciplinari MIUR::Scienze fisiche::ASTRONOMIA E ASTROFISICA | en |
| dc.subject.miur | Scienze fisiche | - |
| dc.subject.isicrui | Categorie ISI-CRUI::Scienze fisiche::Physics | en |
| dc.subject.isicrui | Scienze fisiche | - |
| dc.subject.anagraferoma3 | Scienze fisiche | en |
| dc.relation.volumenumber | 495 | en |
| dc.relation.pagenumber | 421-430 | en |
| dc.identifier.url | http://arxiv.org/abs/0811.1126 | - |
| dc.identifier.doi | 10.1051/0004-6361:200810620 | - |
| dc.relation.issuenumber | 2 | en |
| dc.description.romatrecurrent | Dipartimento di Fisica 'Edoardo Amaldi' | * |
| item.languageiso639-1 | other | - |
| item.fulltext | With Fulltext | - |
| item.grantfulltext | open | - |
| Wuxuu ka dhex muuqdaa ururinnada: | A - Articolo su rivista X_Dipartimento di Fisica 'Edoardo Amaldi' | |
Fayl ku dhex jira qoraalkan:
| Fayl | Sifayn | Baac | Fayl | |
|---|---|---|---|---|
| caixaI.pdf | 700.51 kB | Adobe PDF | Muuji/fur |
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