Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/29904
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Carnall, A. C. | en_US |
dc.contributor.author | McLure, R. J. | en_US |
dc.contributor.author | Dunlop, J. S. | en_US |
dc.contributor.author | Cullen, F. | en_US |
dc.contributor.author | McLeod, D. J. | en_US |
dc.contributor.author | Wild, V. | en_US |
dc.contributor.author | Johnson, B. D. | en_US |
dc.contributor.author | Appleby, S. | en_US |
dc.contributor.author | Davé, R. | en_US |
dc.contributor.author | Amorin, R. | en_US |
dc.contributor.author | BOLZONELLA, MICOL | en_US |
dc.contributor.author | CASTELLANO, MARCO | en_US |
dc.contributor.author | Cimatti, A. | en_US |
dc.contributor.author | CUCCIATI, Olga | en_US |
dc.contributor.author | GARGIULO, ADRIANA | en_US |
dc.contributor.author | GARILLI, BIANCA MARIA ROSA | en_US |
dc.contributor.author | MARCHI, FRANCESCA | en_US |
dc.contributor.author | PENTERICCI, Laura | en_US |
dc.contributor.author | POZZETTI, Lucia | en_US |
dc.contributor.author | Schreiber, C. | en_US |
dc.contributor.author | Talia, M. | en_US |
dc.contributor.author | Zamorani, G. | en_US |
dc.date.accessioned | 2021-01-21T09:39:37Z | - |
dc.date.available | 2021-01-21T09:39:37Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29904 | - |
dc.description.abstract | We present a Bayesian full-spectral-fitting analysis of 75 massive (M_* > 10^{10.3} M_☉ ) UVJ-selected galaxies at redshifts of 1.0 < z < 1.3, combining extremely deep rest-frame ultraviolet spectroscopy from VANDELS with multiwavelength photometry. By the use of a sophisticated physical plus systematic uncertainties model, constructed within the BAGPIPES code, we place strong constraints on the star-formation histories (SFHs) of individual objects. We first constrain the stellar mass versus stellar age relationship, finding a steep trend towards earlier average formation time with increasing stellar mass (downsizing) of 1.48^{+0.34}_{-0.39} Gyr per decade in mass, although this shows signs of flattening at M_* > 10^{11} M_☉ . We show that this is consistent with other spectroscopic studies from 0 < z < 2. This relationship places strong constraints on the AGN-feedback models used in cosmological simulations. We demonstrate that, although the relationships predicted by SIMBA and ILLUSTRISTNG agree well with observations at z = 0.1, they are too shallow at z = 1, predicting an evolution of ≲0.5 Gyr per decade in mass. Secondly, we consider the connections between green-valley, post-starburst, and quiescent galaxies, using our inferred SFH shapes and the distributions of galaxy physical properties on the UVJ diagram. The majority of our lowest-mass galaxies (M_* ∼ 10^{10.5} M_☉ ) are consistent with formation in recent (z < 2), intense starburst events, with time-scales of ≲500 Myr. A second class of objects experience extended star-formation epochs before rapidly quenching, passing through both green-valley and post-starburst phases. The most massive galaxies in our sample are extreme systems: already old by z = 1, they formed at z ∼ 5 and quenched by z = 3. However, we find evidence for their continued evolution through both AGN and rejuvenated star-formation activity. | en_US |
dc.language.iso | eng | en_US |
dc.title | The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stz2544 | en_US |
dc.identifier.scopus | 2-s2.0-85075242938 | en_US |
dc.identifier.isi | 000496922300032 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/490/1/417/5568380 | en_US |
dc.identifier.url | https://arxiv.org/abs/1903.11082 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 490 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 417 | en_US |
dc.relation.numberofpages | 25 | 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 | 2019MNRAS.490..417C | 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 | O.A. Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-3278-4607 | - |
crisitem.author.orcid | 0000-0001-9875-8263 | - |
crisitem.author.orcid | 0000-0002-9336-7551 | - |
crisitem.author.orcid | 0000-0002-3351-1216 | - |
crisitem.author.orcid | 0000-0001-7455-8750 | - |
crisitem.author.orcid | 0000-0002-5694-2545 | - |
crisitem.author.orcid | 0000-0001-8940-6768 | - |
crisitem.author.orcid | 0000-0001-7085-0412 | - |
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Carnall2019.pdf | PDF editoriale | 5.03 MB | Adobe PDF | Visualizza/apri |
Carnall_1903.11082.pdf | arXiv file | 2.1 MB | Adobe PDF | Visualizza/apri |
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