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dc.contributor.authorGarilli, B.
dc.contributor.authorMcLure, R.
dc.contributor.authorPentericci, L.
dc.contributor.authorFranzetti, P.
dc.contributor.authorGargiulo, A.
dc.contributor.authorCarnall, A.
dc.contributor.authorCucciati, O.
dc.contributor.authorIovino, A.
dc.contributor.authorAmorin, R.
dc.contributor.authorBolzonella, M.
dc.contributor.authorBongiorno, A.
dc.contributor.authorCastellano, M.
dc.contributor.authorCimatti, A.
dc.contributor.authorCirasuolo, M.
dc.contributor.authorCullen, F.
dc.contributor.authorDunlop, J.
dc.contributor.authorElbaz, D.
dc.contributor.authorFinkelstein, S.
dc.contributor.authorFontana, A.
dc.contributor.authorFontanot, F.
dc.contributor.authorFumana, M.
dc.contributor.authorGuaita, L.
dc.contributor.authorHartley, W.
dc.contributor.authorJarvis, M.
dc.contributor.authorJuneau, S.
dc.contributor.authorMaccagni, D.
dc.contributor.authorMcLeod, D.
dc.contributor.authorNandra, K.
dc.contributor.authorPompei, E.
dc.contributor.authorPozzetti, L.
dc.contributor.authorScodeggio, M.
dc.contributor.authorTalia, M.
dc.contributor.authorCalabro', A.
dc.contributor.authorCresci, G.
dc.contributor.authorFynbo, J. P. U.
dc.contributor.authorHathi, N. P.
dc.contributor.authorHibon, P.
dc.contributor.authorKoekemoer, A. M.
dc.contributor.authorMagliocchetti, M.
dc.contributor.authorSalvato, M.
dc.contributor.authorVietri, G.
dc.contributor.authorZamorani, G.
dc.contributor.authorAlmaini, O.
dc.contributor.authorBalestra, I.
dc.contributor.authorBardelli, S.
dc.contributor.authorBegley, R.
dc.contributor.authorBrammer, G.
dc.contributor.authorBell, E. F.
dc.contributor.authorBowler, R. A. A.
dc.contributor.authorBrusa, M.
dc.contributor.authorBuitrago, F.
dc.contributor.authorCaputi, C.
dc.contributor.authorCassata, P.
dc.contributor.authorCharlot, S.
dc.contributor.authorCitro, A.
dc.contributor.authorCristiani, S.
dc.contributor.authorCurtis-Lake, E.
dc.contributor.authorDickinson, M.
dc.contributor.authorFazio, G.
dc.contributor.authorFerguson, H. C.
dc.contributor.authorFiore, F.
dc.contributor.authorFranco, M.
dc.contributor.authorGeorgakakis, A.
dc.contributor.authorGiavalisco, M.
dc.contributor.authorGrazian, A.
dc.contributor.authorHamadouche, M.
dc.contributor.authorJung, I.
dc.contributor.authorKim, S.
dc.contributor.authorKhusanova, Y.
dc.contributor.authorFevre, O. Le
dc.contributor.authorLonghetti, M.
dc.contributor.authorLotz, J.
dc.contributor.authorMannucci, F.
dc.contributor.authorMaltby, D.
dc.contributor.authorMatsuoka, K.
dc.contributor.authorMendez-Hernandez, H.
dc.contributor.authorMendez-Abreu, J.
dc.contributor.authorMignoli, M.
dc.contributor.authorMoresco, M.
dc.contributor.authorNonino, M.
dc.contributor.authorPannella, M.
dc.contributor.authorPapovich, C.
dc.contributor.authorPopesso, P.
dc.contributor.authorRoberts-Borsani, G.
dc.contributor.authorRosario, D. J.
dc.contributor.authorSaldana-Lopez, A.
dc.contributor.authorSantini, P.
dc.contributor.authorSaxena, A.
dc.contributor.authorSchaerer, D.
dc.contributor.authorSchreiber, C.
dc.contributor.authorStark, D.
dc.contributor.authorTasca, L. A. M.
dc.contributor.authorThomas, R.
dc.contributor.authorVanzella, E.
dc.contributor.authorWild, V.
dc.contributor.authorWilliams, C.
dc.contributor.authorZucca, E.
dc.date.accessioned2021-03-27T00:07:22Z
dc.date.available2021-03-27T00:07:22Z
dc.date.issued2021-03-26
dc.identifier.citationGarilli , B , McLure , R , Pentericci , L , Franzetti , P , Gargiulo , A , Carnall , A , Cucciati , O , Iovino , A , Amorin , R , Bolzonella , M , Bongiorno , A , Castellano , M , Cimatti , A , Cirasuolo , M , Cullen , F , Dunlop , J , Elbaz , D , Finkelstein , S , Fontana , A , Fontanot , F , Fumana , M , Guaita , L , Hartley , W , Jarvis , M , Juneau , S , Maccagni , D , McLeod , D , Nandra , K , Pompei , E , Pozzetti , L , Scodeggio , M , Talia , M , Calabro' , A , Cresci , G , Fynbo , J P U , Hathi , N P , Hibon , P , Koekemoer , A M , Magliocchetti , M , Salvato , M , Vietri , G , Zamorani , G , Almaini , O , Balestra , I , Bardelli , S , Begley , R , Brammer , G , Bell , E F , Bowler , R A A , Brusa , M , Buitrago , F , Caputi , C , Cassata , P , Charlot , S , Citro , A , Cristiani , S , Curtis-Lake , E , Dickinson , M , Fazio , G , Ferguson , H C , Fiore , F , Franco , M , Georgakakis , A , Giavalisco , M , Grazian , A , Hamadouche , M , Jung , I , Kim , S , Khusanova , Y , Fevre , O L , Longhetti , M , Lotz , J , Mannucci , F , Maltby , D , Matsuoka , K , Mendez-Hernandez , H , Mendez-Abreu , J , Mignoli , M , Moresco , M , Nonino , M , Pannella , M , Papovich , C , Popesso , P , Roberts-Borsani , G , Rosario , D J , Saldana-Lopez , A , Santini , P , Saxena , A , Schaerer , D , Schreiber , C , Stark , D , Tasca , L A M , Thomas , R , Vanzella , E , Wild , V , Williams , C & Zucca , E 2021 , ' The VANDELS ESO public spectroscopic survey : Final Data Release of 2087 spectra and spectroscopic measurements ' , Astronomy & Astrophysics , vol. 647 , A150 . https://doi.org/10.1051/0004-6361/202040059
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 24899228
dc.identifier.otherPURE UUID: 04f46e1b-dacd-40d2-b8aa-e9683e2c4156
dc.identifier.otherArXiv: http://arxiv.org/abs/2101.07645v1
dc.identifier.otherORCID: /0000-0002-3560-8599/work/91300892
dc.identifier.otherScopus: 85103517871
dc.identifier.urihttp://hdl.handle.net/2299/24188
dc.description© ESO 2021. The original publication is available at https://doi.org/10.1051/0004-6361/202040059
dc.description.abstractVANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give a detailed description of sample selection, observations and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at iAB = 25. The high Signal to Noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5{\AA} allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3<Log(M*/Msolar)en
dc.format.extent15
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectastro-ph.GA
dc.subjectastro-ph.CO
dc.titleThe VANDELS ESO public spectroscopic survey : Final Data Release of 2087 spectra and spectroscopic measurementsen
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/202040059
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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