Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/32332
Campo DC | Valore | Lingua |
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dc.contributor.author | Rodríguez-Muñoz, Lucìa | en_US |
dc.contributor.author | RODIGHIERO, GIULIA | en_US |
dc.contributor.author | Pérez-González, P. G. | en_US |
dc.contributor.author | Talia, Margherita | en_US |
dc.contributor.author | BARONCHELLI, Ivano | en_US |
dc.contributor.author | MORSELLI, LAURA | en_US |
dc.contributor.author | Renzini, Alvio | en_US |
dc.contributor.author | Puglisi, Annagrazia | en_US |
dc.contributor.author | GRAZIAN, Andrea | en_US |
dc.contributor.author | ZANELLA, ANITA | en_US |
dc.contributor.author | MANCINI, CHIARA | en_US |
dc.contributor.author | FELTRE, ANNA | en_US |
dc.contributor.author | Romano, M. | en_US |
dc.contributor.author | Vidal García, A. | en_US |
dc.contributor.author | Franceschini, Alberto | en_US |
dc.contributor.author | Alcalde Pampliega, B. | en_US |
dc.contributor.author | CASSATA, PAOLO | en_US |
dc.contributor.author | COSTANTIN, LUCA | en_US |
dc.contributor.author | Domínguez Sánchez, H. | en_US |
dc.contributor.author | Espino-Briones, N. | en_US |
dc.contributor.author | Iani, E. | en_US |
dc.contributor.author | Koekemoer, A. | en_US |
dc.contributor.author | Lumbreras-Calle, A. | en_US |
dc.contributor.author | Rodríguez-Espinosa, J. M. | en_US |
dc.date.accessioned | 2022-06-15T15:47:14Z | - |
dc.date.available | 2022-06-15T15:47:14Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32332 | - |
dc.description.abstract | We use a sample of 706 galaxies, selected as [O II]λ3727 ([O II]) emitters in the Survey for High-z Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with respect to the stellar continuum. The sample includes only galaxies with a counterpart in the infrared and log<SUB>10</SUB>(M<SUB>*</SUB>/M<SUB>⊙</SUB>) > 9, over the redshift interval 0.3 ≲ z ≲ 1.5. Our methodology consists in the comparison of the star formation rates inferred from [O II] and Hα emission lines with a robust quantification of the total star-forming activity (SFR <SUB>TOT</SUB>) that is independently estimated based on both infrared and ultraviolet (UV) luminosities. We obtain $f\, =\, E(B-V)_{\mathrm{stellar}}$/E(B - V)<SUB>nebular</SUB> = 0.69$^{0.71}_{0.69}$ and 0.55$^{0.56}_{0.53}$ for [O II] and Hα, respectively. Our resulting f-factors display a significant positive correlation with the UV attenuation and shallower or not-significant trends with the stellar mass, the SFR<SUB>TOT</SUB>, the distance to the main sequence, and the redshift. Finally, our results favour an average nebular attenuation curve similar in shape to the typical dust curve of local starbursts. | en_US |
dc.language.iso | eng | en_US |
dc.title | Differential attenuation in star-forming galaxies at 0.3 ≲ z ≲ 1.5 in the SHARDS/CANDELS field | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stab3558 | en_US |
dc.identifier.scopus | 2-s2.0-85126354710 | en_US |
dc.identifier.url | http://arxiv.org/abs/2112.01885v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/510/2/2061/6459222 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 510 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2061 | en_US |
dc.relation.lastpage | 2083 | 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 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2022MNRAS.510.2061R | 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 | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0003-0556-2929 | - |
crisitem.author.orcid | 0000-0002-5688-0663 | - |
crisitem.author.orcid | 0000-0001-8600-7008 | - |
crisitem.author.orcid | 0000-0002-4297-0561 | - |
crisitem.author.orcid | 0000-0001-6865-2871 | - |
crisitem.author.orcid | 0000-0001-6820-0015 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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