The VANDELS ESO public spectroscopic survey: Final data release of 2087 spectra and spectroscopic measurements

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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.authorLe Fevre, O.
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.accessioned2025-01-20T23:51:11Z
dc.date.available2025-01-20T23:51:11Z
dc.date.issued2021
dc.description.abstractVANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at i(AB)=25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 angstrom 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-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3 < Log(M-*/M-circle dot) < 11.7.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/202040059
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202040059
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/94783
dc.identifier.wosidWOS:000636920700002
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectgalaxies: distances and redshifts
dc.subjectgalaxies: statistics
dc.subjectgalaxies: fundamental parameters
dc.subjectcosmology: observations
dc.subjectsurveys
dc.subjectcatalogs
dc.titleThe VANDELS ESO public spectroscopic survey: Final data release of 2087 spectra and spectroscopic measurements
dc.typeartículo
dc.volumen647
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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