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Less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS

dc.contributor.authorThomas, R.
dc.contributor.authorPentericci, L.
dc.contributor.authorFèvre, O. Le
dc.contributor.authorKoekemoer, A. M.
dc.contributor.authorCastellano, M.
dc.contributor.authorCimatti, A.
dc.contributor.authorFontanot, F.
dc.contributor.authorGargiulo, A.
dc.contributor.authorGarilli, B.
dc.contributor.authorTalia, M.
dc.contributor.authorAmorín, R.
dc.contributor.authorBardelli, S.
dc.contributor.authorCristiani, S.
dc.contributor.authorCresci, G.
dc.contributor.authorFranco, M.
dc.contributor.authorFynbo, J. P. U.
dc.contributor.authorHathi, N. P.
dc.contributor.authorHibon, P.
dc.contributor.authorKhusanova, Y.
dc.contributor.authorBrun, V. Le
dc.contributor.authorLemaux, B. C.
dc.contributor.authorMannucci, F.
dc.contributor.authorSchaerer, D.
dc.contributor.authorZamorani, G.
dc.contributor.authorZucca, E.
dc.date.accessioned2021-05-07T14:15:01Z
dc.date.available2021-05-07T14:15:01Z
dc.date.issued2021-03-04
dc.identifier.citationThomas , R , Pentericci , L , Fèvre , O L , Koekemoer , A M , Castellano , M , Cimatti , A , Fontanot , F , Gargiulo , A , Garilli , B , Talia , M , Amorín , R , Bardelli , S , Cristiani , S , Cresci , G , Franco , M , Fynbo , J P U , Hathi , N P , Hibon , P , Khusanova , Y , Brun , V L , Lemaux , B C , Mannucci , F , Schaerer , D , Zamorani , G & Zucca , E 2021 , ' Less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS ' , Astronomy & Astrophysics . https://doi.org/10.1051/0004-6361/202038438
dc.identifier.issn0004-6361
dc.identifier.otherArXiv: http://arxiv.org/abs/2103.02946v1
dc.identifier.otherORCID: /0000-0002-3560-8599/work/93471261
dc.identifier.urihttp://hdl.handle.net/2299/24444
dc.description© ESO 2021. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1051/0004-6361/202038438
dc.description.abstractAim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift galaxies. Method. We make use of the VIMOS Ultra Deep Survey and the VANDELS public survey to have an insight into the far UV spectrum of $2.7en
dc.format.extent3530412
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectastro-ph.CO
dc.subjectastro-ph.GA
dc.titleLess and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDSen
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/202038438
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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