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Talia, M.; Schreiber, C.; Garilli, B.; Pentericci, L.; Pozzetti, L.; Zamorani, G.; Cullen, F.; Moresco, M.; Calabrò, A.; Castellano, M.; Fynbo, J. P. U.; Guaita, L.; Marchi, F.; Mascia, S.; McLure, R.; Mignoli, M.; Pompei, E.; Vanzella, E.; Bongiorno, A.; Vietri, G.; Amorín, R. O.; Bolzonella, M.; Carnall, A. C.; Cimatti, A.; Cresci, G.; Cristiani, S.; Cucciati, O.; Dunlop, J. S.; Fontanot, F.; Franzetti, P.; Gargiulo, A.; Hamadouche, M. L.; Hathi, N. P.; Hibon, P.; Iovino, A.; Koekemoer, A. M.; Mannucci, F.; McLeod, D. J.; Saldana-Lopez, A.
Astronomy and astrophysics (Berlin), 10/2023, Letnik: 678Journal Article
VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted ~2100 sources at 1 < z < 6.5 in the CANDELS Chandra Deep-Field South (CDFS) and Ultra-Deep Survey (UDS) fields. In this paper, we present the public release of the spectroscopic measurement catalogues from this survey, featuring emission and absorption line centroids, fluxes, and rest-frame equivalent widths obtained through a Gaussian fit, as well as a number of atomic and molecular indices (e.g. Lick) and continuum breaks (e.g. D4000), and including a correction to be applied to the error spectra. We describe the measurement methods and the validation of the codes that were used.
