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dc.contributor.authorMcLure, R. J.
dc.contributor.authorPentericci, L.
dc.contributor.authorCimatti, A.
dc.contributor.authorDunlop, J. S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFontana, A.
dc.contributor.authorNandra, K.
dc.contributor.authorAmorin, R.
dc.contributor.authorBolzonella, M.
dc.contributor.authorBongiorno, A.
dc.contributor.authorCarnall, A. C.
dc.contributor.authorCastellano, M.
dc.contributor.authorCirasuolo, M.
dc.contributor.authorCucciati, O.
dc.contributor.authorCullen, F.
dc.contributor.authorDe Barros, S.
dc.contributor.authorFinkelstein, S. L.
dc.contributor.authorFontanot, F.
dc.contributor.authorFranzetti, P.
dc.contributor.authorFumana, M.
dc.contributor.authorGargiulo, A.
dc.contributor.authorGarilli, B.
dc.contributor.authorGuaita, L.
dc.contributor.authorHartley, W. G.
dc.contributor.authorIovino, A.
dc.contributor.authorJarvis, M. J.
dc.contributor.authorJuneau, S.
dc.contributor.authorKarman, W.
dc.contributor.authorMaccagni, D.
dc.contributor.authorMarchi, F.
dc.contributor.authorMármol-Queraltó, E.
dc.contributor.authorPompei, E.
dc.contributor.authorPozzetti, L.
dc.contributor.authorScodeggio, M.
dc.contributor.authorSommariva, V.
dc.contributor.authorTalia, M.
dc.contributor.authorAlmaini, O.
dc.contributor.authorBalestra, I.
dc.contributor.authorBardelli, S.
dc.contributor.authorBell, E. F.
dc.contributor.authorBourne, N.
dc.contributor.authorBowler, R. A. A.
dc.contributor.authorBrusa, M.
dc.contributor.authorBuitrago, F.
dc.contributor.authorCaputi, K. I.
dc.contributor.authorCassata, P.
dc.contributor.authorCharlot, S.
dc.contributor.authorCitro, A.
dc.contributor.authorCresci, G.
dc.contributor.authorCristiani, S.
dc.contributor.authorCurtis-Lake, E.
dc.contributor.authorDickinson, M.
dc.contributor.authorFazio, G. G.
dc.contributor.authorFerguson, H. C.
dc.contributor.authorFiore, F.
dc.contributor.authorFranco, M.
dc.contributor.authorFynbo, J. P. U.
dc.contributor.authorGalametz, A.
dc.contributor.authorGeorgakakis, A.
dc.contributor.authorGiavalisco, M.
dc.contributor.authorGrazian, A.
dc.contributor.authorHathi, N. P.
dc.contributor.authorJung, I.
dc.contributor.authorKim, S.
dc.contributor.authorKoekemoer, A. M.
dc.contributor.authorKhusanova, Y.
dc.contributor.authorLe Fèvre, O.
dc.contributor.authorLotz, J. M.
dc.contributor.authorMannucci, F.
dc.contributor.authorMaltby, D. T.
dc.contributor.authorMatsuoka, K.
dc.contributor.authorMcLeod, D. J.
dc.contributor.authorMendez-Hernandez, H.
dc.contributor.authorMendez-Abreu, J.
dc.contributor.authorMignoli, M.
dc.contributor.authorMoresco, M.
dc.contributor.authorMortlock, A.
dc.contributor.authorNonino, M.
dc.contributor.authorPannella, M.
dc.contributor.authorPapovich, C.
dc.contributor.authorPopesso, P.
dc.contributor.authorRosario, D. P.
dc.contributor.authorSalvato, M.
dc.contributor.authorSantini, P.
dc.contributor.authorSchaerer, D.
dc.contributor.authorSchreiber, C.
dc.contributor.authorStark, D. P.
dc.contributor.authorTasca, L. A. M.
dc.contributor.authorThomas, R.
dc.contributor.authorTreu, T.
dc.contributor.authorVanzella, E.
dc.contributor.authorWild, V.
dc.contributor.authorWilliams, C. C.
dc.contributor.authorZamorani, G.
dc.contributor.authorZucca, E.
dc.date.accessioned2018-06-07T10:30:05Z
dc.date.available2018-06-07T10:30:05Z
dc.date.issued2018-09-01
dc.identifier.citationMcLure , R J , Pentericci , L , Cimatti , A , Dunlop , J S , Elbaz , D , Fontana , A , Nandra , K , Amorin , R , Bolzonella , M , Bongiorno , A , Carnall , A C , Castellano , M , Cirasuolo , M , Cucciati , O , Cullen , F , De Barros , S , Finkelstein , S L , Fontanot , F , Franzetti , P , Fumana , M , Gargiulo , A , Garilli , B , Guaita , L , Hartley , W G , Iovino , A , Jarvis , M J , Juneau , S , Karman , W , Maccagni , D , Marchi , F , Mármol-Queraltó , E , Pompei , E , Pozzetti , L , Scodeggio , M , Sommariva , V , Talia , M , Almaini , O , Balestra , I , Bardelli , S , Bell , E F , Bourne , N , Bowler , R A A , Brusa , M , Buitrago , F , Caputi , K I , Cassata , P , Charlot , S , Citro , A , Cresci , G , Cristiani , S , Curtis-Lake , E , Dickinson , M , Fazio , G G , Ferguson , H C , Fiore , F , Franco , M , Fynbo , J P U , Galametz , A , Georgakakis , A , Giavalisco , M , Grazian , A , Hathi , N P , Jung , I , Kim , S , Koekemoer , A M , Khusanova , Y , Le Fèvre , O , Lotz , J M , Mannucci , F , Maltby , D T , Matsuoka , K , McLeod , D J , Mendez-Hernandez , H , Mendez-Abreu , J , Mignoli , M , Moresco , M , Mortlock , A , Nonino , M , Pannella , M , Papovich , C , Popesso , P , Rosario , D P , Salvato , M , Santini , P , Schaerer , D , Schreiber , C , Stark , D P , Tasca , L A M , Thomas , R , Treu , T , Vanzella , E , Wild , V , Williams , C C , Zamorani , G & Zucca , E 2018 , ' The VANDELS ESO spectroscopic survey ' , Monthly Notices of the Royal Astronomical Society , vol. 479 , no. 1 , pp. 25-42 . https://doi.org/10.1093/mnras/sty1213en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 252740426
dc.identifier.otherPURE UUID: 7cc31d9c-95d6-44b7-b093-84c880805c6b
dc.identifier.otherBibCode: 2018arXiv180307414M
dc.identifier.otherBibCode: 2018MNRAS.tmp.1158M
dc.identifier.otherScopus: 85051529204
dc.identifier.otherWOS: 000441295800002
dc.identifier.urihttp://hdl.handle.net/10023/13798
dc.description.abstractVANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO’s Very Large Telescope (VLT). The survey has obtained ultra-deep optical (0.48 < λ < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0 ≤ z ≤ 7.0, over a total area of ≃ 0.2 deg2 centred on the CANDELS UDS and CDFS fields. Based on accurate photometric redshift pre-selection, 85% of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-to-noise ratio (20 < tint < 80 hours), the VANDELS survey targeted: a) bright star-forming galaxies at 2.4 ≤ z ≤ 5.5, b) massive quiescent galaxies at 1.0 ≤ z ≤ 2.5, c) fainter star-forming galaxies at 3.0 ≤ z ≤ 7.0 and d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multi-wavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design and target selection.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2018, the Author(s). This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1093/mnras/sty1213en
dc.subjectSurveysen
dc.subjectGalaxies: high-redshiften
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: star formationen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe VANDELS ESO spectroscopic surveyen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/sty1213
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2018arXiv180307414Men
dc.identifier.urlhttps://arxiv.org/abs/1803.07414en


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