Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26534
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Malavasi, N. | en_US |
dc.contributor.author | Arnouts, S. | en_US |
dc.contributor.author | Vibert, D. | en_US |
dc.contributor.author | de la Torre, S. | en_US |
dc.contributor.author | Moutard, T. | en_US |
dc.contributor.author | Pichon, C. | en_US |
dc.contributor.author | Davidzon, I. | en_US |
dc.contributor.author | Kraljic, K. | en_US |
dc.contributor.author | BOLZONELLA, MICOL | en_US |
dc.contributor.author | Guzzo, L. | en_US |
dc.contributor.author | GARILLI, BIANCA MARIA ROSA | en_US |
dc.contributor.author | SCODEGGIO, MARCO | en_US |
dc.contributor.author | GRANETT, Benjamin Rudolph | en_US |
dc.contributor.author | ABBAS, Ummi | en_US |
dc.contributor.author | Adami, C. | en_US |
dc.contributor.author | BOTTINI, DARIO | en_US |
dc.contributor.author | CAPPI, Alberto | en_US |
dc.contributor.author | CUCCIATI, Olga | en_US |
dc.contributor.author | FRANZETTI, PAOLO | en_US |
dc.contributor.author | Fritz, A. | en_US |
dc.contributor.author | IOVINO, Angela | en_US |
dc.contributor.author | Krywult, J. | en_US |
dc.contributor.author | Le Brun, V. | en_US |
dc.contributor.author | Le Fèvre, O. | en_US |
dc.contributor.author | Maccagni, D. | en_US |
dc.contributor.author | Małek, K. | en_US |
dc.contributor.author | Marulli, F. | en_US |
dc.contributor.author | POLLETTA, MARIA DEL CARMEN | en_US |
dc.contributor.author | Pollo, A. | en_US |
dc.contributor.author | Tasca, L. | en_US |
dc.contributor.author | Tojeiro, R. | en_US |
dc.contributor.author | VERGANI, DANIELA | en_US |
dc.contributor.author | ZANICHELLI, Alessandra | en_US |
dc.contributor.author | Bel, J. | en_US |
dc.contributor.author | Branchini, Enzo Franco | en_US |
dc.contributor.author | Coupon, J. | en_US |
dc.contributor.author | DE LUCIA, GABRIELLA | en_US |
dc.contributor.author | Dubois, Y. | en_US |
dc.contributor.author | Hawken, A. | en_US |
dc.contributor.author | Ilbert, O. | en_US |
dc.contributor.author | Laigle, C. | en_US |
dc.contributor.author | Moscardini, L. | en_US |
dc.contributor.author | Sousbie, T. | en_US |
dc.contributor.author | Treyer, M. | en_US |
dc.contributor.author | Zamorani, G. | en_US |
dc.date.accessioned | 2020-07-21T06:04:37Z | - |
dc.date.available | 2020-07-21T06:04:37Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26534 | - |
dc.description.abstract | We present the first quantitative detection of large-scale filamentary structure at z ≃ 0.7 in the large cosmological volume probed by the VIMOS Public Extragalactic Redshift Survey (VIPERS). We use simulations to show the capability of VIPERS to recover robust topological features in the galaxy distribution, in particular the filamentary network. We then investigate how galaxies with different stellar masses and stellar activities are distributed around the filaments, and find a significant segregation, with the most massive or quiescent galaxies being closer to the filament axis than less massive or active galaxies. The signal persists even after downweighting the contribution of peak regions. Our results suggest that massive and quiescent galaxies assemble their stellar mass through successive mergers during their migration along filaments towards the nodes of the cosmic web. On the other hand, low-mass star-forming galaxies prefer the outer edge of filaments, a vorticity-rich region dominated by smooth accretion, as predicted by the recent spin alignment theory. This emphasizes the role of large-scale cosmic flows in shaping galaxy properties. | en_US |
dc.language.iso | eng | en_US |
dc.title | The VIMOS Public Extragalactic Redshift Survey (VIPERS): galaxy segregation inside filaments at z ≃ 0.7 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw2864 | en_US |
dc.identifier.scopus | 2-s2.0-85014860832 | en_US |
dc.identifier.isi | 000395170200005 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/465/4/3817/2420717 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 465 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 3817 | en_US |
dc.relation.lastpage | 3822 | en_US |
dc.relation.numberofpages | 7 | 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 | en_US |
dc.identifier.adsbibcode | 2017MNRAS.465.3817M | 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 | IASF Milano | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0003-3278-4607 | - |
crisitem.author.orcid | 0000-0001-7455-8750 | - |
crisitem.author.orcid | 0000-0002-2282-5850 | - |
crisitem.author.orcid | 0000-0003-2694-9284 | - |
crisitem.author.orcid | 0000-0002-5076-766X | - |
crisitem.author.orcid | 0000-0001-6917-041X | - |
crisitem.author.orcid | 0000-0002-9200-7167 | - |
crisitem.author.orcid | 0000-0002-9336-7551 | - |
crisitem.author.orcid | 0000-0002-6986-0127 | - |
crisitem.author.orcid | 0000-0001-6958-0304 | - |
crisitem.author.orcid | 0000-0001-7411-5386 | - |
crisitem.author.orcid | 0000-0003-0898-2216 | - |
crisitem.author.orcid | 0000-0002-2893-023X | - |
crisitem.author.orcid | 0000-0002-6220-9104 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Malavasi2017.pdf | PDF editoriale | 3.48 MB | Adobe PDF | View/Open |
Malavasi_1611.07045.pdf | preprint | 1.56 MB | Adobe PDF | View/Open |
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