Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/29077
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | LANZUISI, Giorgio | en_US |
dc.contributor.author | Civano, F. | en_US |
dc.contributor.author | MARCHESI, STEFANO | en_US |
dc.contributor.author | COMASTRI, Andrea | en_US |
dc.contributor.author | Brusa, M. | en_US |
dc.contributor.author | GILLI, Roberto | en_US |
dc.contributor.author | Vignali, C. | en_US |
dc.contributor.author | Zamorani, G. | en_US |
dc.contributor.author | Brightman, M. | en_US |
dc.contributor.author | Griffiths, R. E. | en_US |
dc.contributor.author | Koekemoer, A. M. | en_US |
dc.date.accessioned | 2020-12-22T09:22:47Z | - |
dc.date.available | 2020-12-22T09:22:47Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29077 | - |
dc.description.abstract | The existence of a large population of Compton thick (CT; N<SUB>H</SUB> > 10<SUP>24</SUP> cm<SUP>-2</SUP>) active galactic nuclei (AGN) is a key ingredient of most cosmic X-ray background synthesis models. However, direct identification of these sources, especially at high redshift, is difficult due to flux suppression and complex spectral shape produced by CT obscuration. We explored the Chandra Cosmological Evolution Survey (COSMOS) Legacy point source catalogue, comprising 1855 sources to select, via X-ray spectroscopy, a large sample of CT candidates at high redshift. Adopting a physical model to reproduce the toroidal absorber and a Monte-Carlo sampling method, we selected 67 individual sources with > 5 per cent probability of being CT, in the redshift range 0.04 ≲ z ≲ 3.5. The sum of the probabilities above N<SUB>H</SUB> > 10<SUP>24</SUP> cm<SUP>-2</SUP> gives a total of 41.9 effective CT, corrected for classification bias. We derive number counts in the 2-10 keV band in three redshift bins. The observed log N-log S is consistent with an increase of the intrinsic CT fraction (f<SUB>CT</SUB>) from ∼0.30 to ∼0.55 from low to high redshift. When rescaled to a common luminosity (log(L<SUB>X</SUB>/ erg s<SUP>-1</SUP>) = 44.5), we find an increase from f<SUB>CT</SUB> = 0.19_{-0.06}^{+0.07} to 0.30_{-0.08}^{+0.10} and f<SUB>CT</SUB> = 0.49_{-0.11}^{+0.12} from low to high z. This evolution can be parametrized as f<SUB>CT</SUB> = 0.11_{-0.04}^{+0.05}(1+z)^{1.11± 0.13}. Thanks to Hubble Space Telescope-Advanced Camera for Surveys deep imaging, we find that the fraction of CT AGN in mergers/interacting systems increases with luminosity and redshift and is significantly higher than for non-CT AGN hosts. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Chandra COSMOS Legacy Survey: Compton thick AGN at high redshift | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty2025 | en_US |
dc.identifier.scopus | 2-s2.0-85055323149 | en_US |
dc.identifier.isi | 000449614800088 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/full_html/2019/01/aa32383-17/aa32383-17.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 480 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2578 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018MNRAS.480.2578L | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | 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 | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-9094-0984 | - |
crisitem.author.orcid | 0000-0001-5544-0749 | - |
crisitem.author.orcid | 0000-0003-3451-9970 | - |
crisitem.author.orcid | 0000-0001-8121-6177 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
sty2025.pdf | PDF editoriale | 4.2 MB | Adobe PDF | Visualizza/apri |
Page view(s)
66
controllato il 5-ago-2024
Download(s)
22
controllato il 5-ago-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.