Cox, N. L. J.N. L. J.Cox0000-0003-0602-6669Cami, J.J.CamiFarhang, A.A.FarhangSmoker, J.J.SmokerMonreal-Ibero, A.A.Monreal-IberoLallement, R.R.LallementSarre, P. J.P. J.SarreMarshall, C. C. M.C. C. M.MarshallSmith, K. T.K. T.SmithEvans, C. J.C. J.EvansRoyer, P.P.RoyerLinnartz, H.H.LinnartzCordiner, M. A.M. A.CordinerJoblin, C.C.Joblinvan Loon, J. T.J. T.van LoonFoing, B. H.B. H.FoingBhatt, N. H.N. H.BhattBron, E.E.BronElyajouri, M.M.Elyajouride Koter, A.A.de KoterEhrenfreund, P.P.EhrenfreundJavadi, A.A.JavadiKaper, L.L.KaperKhosroshadi, H. G.H. G.KhosroshadiLaverick, M.M.LaverickLe Petit, F.F.Le PetitMULAS, GiacomoGiacomoMULASRoueff, E.E.RoueffSalama, F.F.SalamaSpaans, M.M.Spaans2022-03-292022-03-292018http://hdl.handle.net/20.500.12386/32007We constructed a statistically representative survey sample that probes a wide range of interstellar environment parameters including reddening E(B-V), visual extinction A<SUB>V</SUB>, total-to-selective extinction ratio R<SUB>V</SUB>, and molecular hydrogen fraction f<SUB>H2</SUB>. <P />EDIBLES provides the community with optical (~305-1042nm) spectra at high spectral resolution (R~70000 in the blue arm and 100000 in the red arm) and high signal-to-noise (S/N; median value ~500-1000), for a statistically significant sample of interstellar sightlines. Many of the >100 sightlines included in the survey already have auxiliary available ultraviolet, infrared and/or polarisation data on the dust and gas components. <P />(2 data files).enDatabase10.26093/cds/vizier.36060076https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/606/A762018yCat..36060076CFIS/05 - ASTRONOMIA E ASTROFISICA