Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31478
DC Field | Value | Language |
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dc.contributor.author | Old, Lyndsay J. | en_US |
dc.contributor.author | Balogh, Michael L. | en_US |
dc.contributor.author | van der Burg, Remco F. J. | en_US |
dc.contributor.author | BIVIANO, ANDREA | en_US |
dc.contributor.author | Yee, Howard K. C. | en_US |
dc.contributor.author | Pintos-Castro, Irene | en_US |
dc.contributor.author | Webb, Kristi | en_US |
dc.contributor.author | Muzzin, Adam | en_US |
dc.contributor.author | Rudnick, Gregory | en_US |
dc.contributor.author | Vulcani, Benedetta | en_US |
dc.contributor.author | Poggianti, Bianca | en_US |
dc.contributor.author | Cooper, Michael | en_US |
dc.contributor.author | Zaritsky, Dennis | en_US |
dc.contributor.author | Cerulo, Pierluigi | en_US |
dc.contributor.author | Wilson, Gillian | en_US |
dc.contributor.author | Chan, Jeffrey C. C. | en_US |
dc.contributor.author | Lidman, Chris | en_US |
dc.contributor.author | McGee, Sean | en_US |
dc.contributor.author | Demarco, Ricardo | en_US |
dc.contributor.author | Forrest, Ben | en_US |
dc.contributor.author | DE LUCIA, GABRIELLA | en_US |
dc.contributor.author | Gilbank, David | en_US |
dc.contributor.author | Kukstas, Egidijus | en_US |
dc.contributor.author | McCarthy, Ian G. | en_US |
dc.contributor.author | Jablonka, Pascale | en_US |
dc.contributor.author | Nantais, Julie | en_US |
dc.contributor.author | Noble, Allison | en_US |
dc.contributor.author | Reeves, Andrew M. M. | en_US |
dc.contributor.author | Shipley, Heath | en_US |
dc.date.accessioned | 2022-02-25T11:28:13Z | - |
dc.date.available | 2022-02-25T11:28:13Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31478 | - |
dc.description.abstract | We present results on the environmental dependence of the star-forming galaxy main sequence in 11 galaxy cluster fields at 1.0 < z < 1.5 from the Gemini Observations of Galaxies in Rich Early Environments Survey (GOGREEN) survey. We use a homogeneously selected sample of field and cluster galaxies whose membership is derived from dynamical analysis. Using [O<SUB>II</SUB>]-derived star formation rates (SFRs), we find that cluster galaxies have suppressed SFRs at fixed stellar mass in comparison to their field counterparts by a factor of 1.4 ± 0.1 (∼3.3σ) across the stellar mass range: 9.0 < log (M<SUB>*</SUB>/M<SUB>⊙</SUB>) < 11.2. We also find that this modest suppression in the cluster galaxy star-forming main sequence is mass and redshift dependent: the difference between cluster and field increases towards lower stellar masses and lower redshift. When comparing the distribution of cluster and field galaxy SFRs to the star-forming main sequence, we find an overall shift towards lower SFRs in the cluster population, and note the absence of a tail of high SFR galaxies as seen in the field. Given this observed suppression in the cluster galaxy star-forming main sequence, we explore the implications for several scenarios such as formation time differences between cluster and field galaxies, and environmentally induced star formation quenching and associated time-scales. | en_US |
dc.language.iso | eng | en_US |
dc.title | The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/staa579 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/493/4/5987/5780231?login=true | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 493 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 5987 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 29 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | 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 | 2020MNRAS.493.5987O | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-0857-0732 | - |
crisitem.author.orcid | 0000-0003-0980-1499 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
gogreen_old.pdf | Pdf editoriale | 4.91 MB | Adobe PDF | View/Open |
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