INNO, LAURALAURAINNO0000-0002-0271-2664Matsunaga, N.N.Matsunaga0000-0001-6342-9662Romaniello, M.M.RomanielloBono, G.G.BonoMonson, A.A.MonsonFerraro, I.I.FerraroIannicola, G.G.IannicolaPersson, E.E.PerssonBuonanno, R.R.BuonannoFreedman, W.W.FreedmanGieren, W.W.GierenGroenewegen, M. A. T.M. A. T.GroenewegenIta, Y.Y.ItaLaney, C. D.C. D.LaneyLemasle, B.B.LemasleMadore, B. F.B. F.MadoreNagayama, T.T.NagayamaNakada, Y.Y.NakadaNONINO, MarioMarioNONINOPietrzynski, G.G.PietrzynskiPrimas, F.F.PrimasScowcroft, V.V.ScowcroftSoszynski, I.I.SoszynskiTanabe, T.T.TanabeUdalski, A.A.Udalski2020-06-252020-06-252015http://hdl.handle.net/20.500.12386/26214Our analysis is based on the largest available sample of fundamental-mode Cepheids with well-covered light-curves in the NIR and in optical (V, I) bands. This sample covers a very broad period range (1-100 days). We collected J, H, and KS band observations from four different data sets: Laney & Stobie (1992A&AS...93...93L, 51) and Monson & Pierce (2011ApJS..193...12M, 131) for Galactic Cepheids, Persson et al. (2004AJ....128.2239P, 92) for LMC Cepheids, and the IRSF survey catalog for ~500 Small Magellanic Cloud (SMC) Cepheids. (2 data files).enDatabasehttps://doi.org//10.26093/cds/vizier.35760030https://cdsarc.unistra.fr/viz-bin/cat/J/A+A/576/A302015yCat..35760030IFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation