Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30097
DC Field | Value | Language |
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dc.contributor.author | Wang, L. | en_US |
dc.contributor.author | Gao, F. | en_US |
dc.contributor.author | Duncan, K. J. | en_US |
dc.contributor.author | Williams, W. L. | en_US |
dc.contributor.author | Rowan-Robinson, M. | en_US |
dc.contributor.author | Sabater, J. | en_US |
dc.contributor.author | Shimwell, T. W. | en_US |
dc.contributor.author | BONATO, MATTEO | en_US |
dc.contributor.author | Calistro-Rivera, G. | en_US |
dc.contributor.author | Chyży, K. T. | en_US |
dc.contributor.author | Farrah, D. | en_US |
dc.contributor.author | Gürkan, G. | en_US |
dc.contributor.author | Hardcastle, M. J. | en_US |
dc.contributor.author | McCheyne, I. | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | READ, SHAUN CONISBEE | en_US |
dc.contributor.author | Röttgering, H. J. A. | en_US |
dc.contributor.author | Smith, D. J. B. | en_US |
dc.date.accessioned | 2021-01-29T09:29:44Z | - |
dc.date.available | 2021-01-29T09:29:44Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30097 | - |
dc.description.abstract | <BR /> Aims: We aim to study the far-infrared radio correlation (FIRC) at 150 MHz in the local Universe (at a median redshift ⟨z⟩∼0.05) and improve the use of the rest-frame 150 MHz luminosity, L<SUB>150</SUB>, as a star-formation rate (SFR) tracer, which is unaffected by dust extinction. <BR /> Methods: We cross-match the 60 μm selected Revised IRAS Faint Source Survey Redshift (RIFSCz) catalogue and the 150 MHz selected LOFAR value-added source catalogue in the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Spring Field. We estimate L<SUB>150</SUB> for the cross-matched sources and compare it with the total infrared (IR) luminosity, L<SUB>IR</SUB>, and various SFR tracers. <BR /> Results: We find a tight linear correlation between log L<SUB>150</SUB> and log L<SUB>IR</SUB> for star-forming galaxies, with a slope of 1.37. The median q<SUP>IR</SUP> value (defined as the logarithm of the L<SUB>IR</SUB> to L<SUB>150</SUB> ratio) and its rms scatter of our main sample are 2.14 and 0.34, respectively. We also find that log L<SUB>150</SUB> correlates tightly with the logarithm of SFR derived from three different tracers, i.e., SFR<SUB>Hα</SUB> based on the Hα line luminosity, SFR<SUB>60</SUB> based on the rest-frame 60 μm luminosity and SFR<SUB>IR</SUB> based on L<SUB>IR</SUB>, with a scatter of 0.3 dex. Our best-fit relations between L<SUB>150</SUB> and these SFR tracers are, log L<SUB>150</SUB> (L<SUB>☉</SUB>) = 1.35(±0.06) × log SFR<SUB>Hα</SUB> (M<SUB>☉</SUB> yr<SUP>-1</SUP>) + 3.20(±0.06), log L<SUB>150</SUB> (L<SUB>☉</SUB>) = 1.31(±0.05) × log SFR<SUB>60</SUB> (M<SUB>☉</SUB> yr<SUP>-1</SUP>) + 3.14(±0.06), and log L<SUB>150</SUB> (L<SUB>☉</SUB>) = 1.37 (±0.05) × log SFR<SUB>IR</SUB> (M<SUB>☉</SUB> yr<SUP>-1</SUP>) + 3.09(±0.05), which show excellent agreement with each other. | en_US |
dc.language.iso | eng | en_US |
dc.title | A LOFAR-IRAS cross-match study: the far-infrared radio correlation and the 150 MHz luminosity as a star-formation rate tracer | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201935913 | en_US |
dc.identifier.scopus | 2-s2.0-85089875385 | en_US |
dc.identifier.isi | 000515096100001 | en_US |
dc.identifier.url | http://arxiv.org/abs/1909.04489v1 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/full_html/2019/11/aa35913-19/aa35913-19.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 631 | en_US |
dc.relation.firstpage | A109 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | 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 | 2019A&A...631A.109W | 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.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0001-9139-2342 | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
crisitem.author.orcid | 0000-0001-9188-9359 | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Wang+19.pdf | postprint | 1.27 MB | Adobe PDF | View/Open |
aa35913-19.pdf | Pdf editoriale | 640.46 kB | Adobe PDF | View/Open |
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