Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31996
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | MARCHESI, STEFANO | en_US |
dc.contributor.author | MIGNOLI, Marco | en_US |
dc.contributor.author | GILLI, Roberto | en_US |
dc.contributor.author | PECA, ALESSANDRO | en_US |
dc.contributor.author | BOLZONELLA, MICOL | en_US |
dc.contributor.author | NANNI, RICCARDO | en_US |
dc.contributor.author | Marianna Annunziatella | en_US |
dc.contributor.author | BALMAVERDE, Barbara | en_US |
dc.contributor.author | Brusa, Marcella | en_US |
dc.contributor.author | CALURA, Francesco | en_US |
dc.contributor.author | CASSARA, LETIZIA PASQUA | en_US |
dc.contributor.author | Marco Chiaberge | en_US |
dc.contributor.author | COMASTRI, Andrea | en_US |
dc.contributor.author | CUSANO, FELICE | en_US |
dc.contributor.author | Quirino D'Amato | en_US |
dc.contributor.author | Kazushi Iwasawa | en_US |
dc.contributor.author | LANZUISI, Giorgio | en_US |
dc.contributor.author | Danilo Marchesini | en_US |
dc.contributor.author | Takahiro Morishita | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | ROSSI, Andrea | en_US |
dc.contributor.author | TOZZI, Paolo | en_US |
dc.contributor.author | VIGNALI, CRISTIAN | en_US |
dc.contributor.author | Vito, Fabio | en_US |
dc.contributor.author | ZAMORANI, Giovanni | en_US |
dc.contributor.author | Colin Norman | en_US |
dc.date.accessioned | 2022-03-29T09:35:22Z | - |
dc.date.available | 2022-03-29T09:35:22Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31996 | - |
dc.description.abstract | We publicly release the spectroscopic and photometric redshift catalog of the sources detected with Chandra in the field of the $z$=6.3 quasar SDSS J1030+0525. This is currently the fifth deepest X-ray field, and reaches a 0.5-2 keV flux limit $f_{\rm 0.5-2}$=6$\times$10$^{-17}$ erg s$^{-1}$ cm$^{-2}$. By using two independent methods, we measure a photometric redshift for 243 objects, while 123 (51%) sources also have a spectroscopic redshift, 110 of which coming from an INAF-Large Binocular Telescope (LBT) Strategic Program. We use the spectroscopic redshifts to determine the quality of the photometric ones, and find it in agreement with that of other X-ray surveys which used a similar number of photometric data-points. In particular, we measure a sample normalized median absolute deviation $\sigma_{NMAD}$=1.48||$z_{phot}$-$z_{spec}$||/(1+$z_{spec}$)=0.065. We use these new spectroscopic and photometric redshifts to study the properties of the Chandra J1030 field. We observe several peaks in our spectroscopic redshift distribution between $z$=0.15 and $z$=1.5, and find that the sources in each peak are often distributed across the whole Chandra field of view. This evidence confirms that X-ray selected AGN can efficiently track large-scale structures over physical scales of several Mpc. Finally, we computed the Chandra J1030 $z>$3 number counts: while the spectroscopic completeness at high-redshift of our sample is limited, our results point towards a potential source excess at $z\geq$4, which we plan to either confirm or reject in the near future with dedicated spectroscopic campaigns. | en_US |
dc.language.iso | eng | en_US |
dc.title | Redshift identification of X-ray selected active galactic nuclei in the J1030 field: searching for large-scale structures and high-redshift sources | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/202141416 | en_US |
dc.identifier.scopus | 2-s2.0-85121272821 | en_US |
dc.identifier.url | http://arxiv.org/abs/2109.08162v1 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2021/12/aa41416-21/aa41416-21.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 656 | en_US |
dc.relation.firstpage | A117 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 26 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | JPN | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021A&A...656A.117M | 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 | 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 | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-5544-0749 | - |
crisitem.author.orcid | 0000-0002-9087-2835 | - |
crisitem.author.orcid | 0000-0001-8121-6177 | - |
crisitem.author.orcid | 0000-0003-3278-4607 | - |
crisitem.author.orcid | 0000-0002-0690-0638 | - |
crisitem.author.orcid | 0000-0002-6175-0871 | - |
crisitem.author.orcid | 0000-0001-5760-089X | - |
crisitem.author.orcid | 0000-0003-3451-9970 | - |
crisitem.author.orcid | 0000-0003-2910-6565 | - |
crisitem.author.orcid | 0000-0001-9094-0984 | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
crisitem.author.orcid | 0000-0002-8860-6538 | - |
crisitem.author.orcid | 0000-0003-3096-9966 | - |
crisitem.author.orcid | 0000-0003-0680-9305 | - |
crisitem.author.orcid | 0000-0002-2318-301X | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
aa41416-21.pdf | PDF editoriale | 7.37 MB | Adobe PDF | Visualizza/apri |
2109.08162.pdf | preprint | 7.2 MB | Adobe PDF | Visualizza/apri |
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