Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31528
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Giulietti, M. | en_US |
dc.contributor.author | MASSARDI, MARCELLA | en_US |
dc.contributor.author | Lapi, A. | en_US |
dc.contributor.author | BONATO, MATTEO | en_US |
dc.contributor.author | Enia, A. F. M. | en_US |
dc.contributor.author | Negrello, M. | en_US |
dc.contributor.author | D'Amato, Q. | en_US |
dc.contributor.author | Behiri, M. | en_US |
dc.contributor.author | De Zotti, G. | en_US |
dc.date.accessioned | 2022-03-08T11:27:00Z | - |
dc.date.available | 2022-03-08T11:27:00Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31528 | - |
dc.description.abstract | We investigate the radio-far infrared (FIR) correlation for a sample of $28$ bright high-redshift ($1 \lesssim z \lesssim 4$) star-forming galaxies selected in the FIR from the Herschel-ATLAS fields as candidates to be strongly gravitationally lensed. The radio information comes either from high sensitivity dedicated ATCA observations at $2.1$ GHz or from cross-matches with the FIRST survey at $1.4$ GHz. By taking advantage of source brightness possibly enhanced by lensing magnification, we identify a weak evolution with redshift out to $z\lesssim 4$ of the FIR-to-radio luminosity ratio $q_{\rm FIR}$. We also find that the $q_{\rm FIR}$ parameter as a function of the radio power $L_{1.4\,\rm GHz}$ displays a clear decreasing trend, similarly to what is observed for optically/radio selected lensed quasars found in literature, yet covering a complementary region in the $q_{\rm FIR}-L_{1.4\,\rm GHz}$ diagram. We interpret such a behavior in the framework of an in-situ galaxy formation scenario, as a result of the transition from an early dust-obscured star-forming phase (mainly pinpointed by our FIR selection) to a late radio-loud quasar phase (preferentially sampled by the optical/radio selection). | en_US |
dc.language.iso | eng | en_US |
dc.title | The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stac145 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/511/1/1408/6515977?redirectedFrom=fulltext&login=false | en_US |
dc.identifier.url | http://arxiv.org/abs/2201.06466v2 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.type.referee | REF_1 | 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.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.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0002-0375-8330 | - |
crisitem.author.orcid | 0000-0001-9139-2342 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
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2201.06466.pdf | preprint | 7.39 MB | Adobe PDF | Visualizza/apri |
stac145.pdf | Pdf editoriale | 1.96 MB | Adobe PDF | Visualizza/apri |
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