Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model : I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering

2011
journal article
article
cris.lastimport.scopus2024-04-26T01:18:16Z
dc.affiliationWydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomicznepl
dc.contributor.authorde la Torre, S.pl
dc.contributor.authorMeneux, B.pl
dc.contributor.authorDe Lucia, G.pl
dc.contributor.authorBlaizot, J.pl
dc.contributor.authorLe Fèvre, O.pl
dc.contributor.authorGarilli, B.pl
dc.contributor.authorCucciati, O.pl
dc.contributor.authorMellier, Y.pl
dc.contributor.authorPollo, Agnieszka - 131503 pl
dc.contributor.authorAbbas, U.pl
dc.contributor.authorBottini, D.pl
dc.contributor.authorLe Brun, V.pl
dc.contributor.authorMaccagni, D.pl
dc.contributor.authorScodeggio, M.pl
dc.contributor.authorTresse, L.pl
dc.contributor.authorVettolani, G.pl
dc.contributor.authorZanichelli, A.pl
dc.contributor.authorAdami, C.pl
dc.contributor.authorArnouts, S.pl
dc.contributor.authorBardelli, S.pl
dc.contributor.authorBolzonella, M.pl
dc.contributor.authorCappi, A.pl
dc.contributor.authorCharlot, S.pl
dc.contributor.authorCiliegi, P.pl
dc.contributor.authorContini, T.pl
dc.contributor.authorFoucaud, S.pl
dc.contributor.authorFranzetti, P.pl
dc.contributor.authorGavignaud, I.pl
dc.contributor.authorGuzzo, L.pl
dc.contributor.authorIlbert, O.pl
dc.contributor.authorIovino, A.pl
dc.contributor.authorMcCracken, H. J.pl
dc.contributor.authorMarinoni, C.pl
dc.contributor.authorMazure, A.pl
dc.contributor.authorMerighi, R.pl
dc.contributor.authorPaltani, S.pl
dc.contributor.authorPelló, R.pl
dc.contributor.authorPozzetti, L.pl
dc.contributor.authorVergani, D.pl
dc.contributor.authorZamorani, G.pl
dc.contributor.authorZucca, E.pl
dc.date.accessioned2019-02-14T08:59:17Z
dc.date.available2019-02-14T08:59:17Z
dc.date.issued2011pl
dc.date.openaccess12
dc.description.accesstimepo opublikowaniu
dc.description.additionalReproduced with permission from Astronomy & Astrophysics, © ESOpl
dc.description.versionostateczna wersja wydawcy
dc.description.volume525pl
dc.identifier.articleidA125pl
dc.identifier.doi10.1051/0004-6361/201015540pl
dc.identifier.eissn1432-0746pl
dc.identifier.issn0004-6361pl
dc.identifier.projectROD UJ / OPpl
dc.identifier.urihttps://ruj.uj.edu.pl/xmlui/handle/item/68340
dc.languageengpl
dc.language.containerengpl
dc.rightsUdzielam licencji. Uznanie autorstwa - Użycie niekomercyjne - Na tych samych warunkach 4.0 Międzynarodowa*
dc.rights.licenceOTHER
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.pl*
dc.share.typeotwarte czasopismo
dc.subject.encosmology: observationspl
dc.subject.enlarge-scale structure of Universepl
dc.subject.engalaxies: evolutionpl
dc.subject.engalaxies: high-redshiftpl
dc.subject.engalaxies: statisticspl
dc.subtypeArticlepl
dc.titleComparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model : I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clusteringpl
dc.title.journalAstronomy & Astrophysicspl
dc.typeJournalArticlepl
dspace.entity.typePublication
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