Hamuy, M.M.HamuyPhillips, M. M.M. M.PhillipsSuntzeff, N. B.N. B.SuntzeffSchommer, R. A.R. A.SchommerMaza, J.J.MazaAntezan, A. R.A. R.AntezanWischnjewsky, M.M.WischnjewskyValladares, G.G.ValladaresMuena, C.C.MuenaGonzales, L. E.L. E.GonzalesAviles, R.R.AvilesWells, L. A.L. A.WellsSmith, R. C.R. C.SmithNavarrete, M.M.NavarreteCovarrubias, R.R.CovarrubiasWilliger, G. M.G. M.WilligerWalker, A. R.A. R.WalkerLayden, A. C.A. C.LaydenElias, J. H.J. H.EliasBaldwin, J. A.J. A.BaldwinHernandez, M.M.HernandezTirado, H.H.TiradoUgarte, P.P.UgarteElston, R.R.ElstonSaavedra, N.N.SaavedraBarrientos, F.F.BarrientosCOSTA, ELIAELIACOSTALira, P.P.LiraRuiz, M. T.M. T.RuizAnguita, C.C.AnguitaGomez, X.X.GomezOrtiz, P.P.OrtizDELLA VALLE, MassimoMassimoDELLA VALLEDanziger, J.J.DanzigerStorm, J.J.StormKim, Y. -C.Y. -C.KimBailyn, C.C.BailynRubenstein, E. P.E. P.RubensteinTucker, D.D.TuckerCersosimo, S.S.CersosimoMendez, R. A.R. A.MendezSiciliano, L.L.SicilianoSherry, W.W.SherryChaboyer, B.B.ChaboyerKoopmann, R. A.R. A.KoopmannGeisler, D.D.GeislerSarajedini, A.A.SarajediniDey, A.A.DeyTyson, N.N.TysonRich, R. M.R. M.RichGal, R.R.GalLamontagne, R.R.LamontagneCaldwell, N.N.CaldwellGuhathakurta, P.P.GuhathakurtaPhillips, A. C.A. C.PhillipsSzkody, P.P.SzkodyProsser, C.C.ProsserHo, L. C.L. C.HoMcMahan, R.R.McMahanBaggley, G.G.BaggleyCheng, K. -P.K. -P.ChengHavlen, R.R.HavlenWakamatsu, K.K.WakamatsuJanes, K.K.JanesMalkan, M.M.MalkanBaganoff, F.F.BaganoffSeitzer, P.P.SeitzerShara, M.M.SharaSturch, C.C.SturchHesser, J.J.HesserHartigan, P.P.HartiganHughes, J.J.HughesWelch, D.D.WelchWilliams, T. B.T. B.WilliamsFerguson, H.H.FergusonFrancis, P. J.P. J.FrancisFrench, L.L.FrenchBolte, M.M.BolteRoth, J.J.RothOdewahn, S.S.OdewahnHowell, S.S.HowellKrzeminski, W.W.Krzeminski2022-10-042022-10-0419960004-6256http://hdl.handle.net/20.500.12386/32690BV(RI)_KC_ light curves are presented for 27 type Ia supernovae discovered during the course of the Calan/Tololo Survey and for two other SNe Ia observed during the same period. Estimates of the maximum light magnitudes in the B, V, and I bands and the initial decline rate parameter {DELTA}m_15_(B) are also given.STAMPAenBVRI Light Curves for 29 Type IA SupernovaeArticle10.1086/1181922-s2.0-5844323584https://ui.adsabs.harvard.edu/abs/1996AJ....112.2408H/abstracthttp://arxiv.org/abs/astro-ph/9609064v11996AJ....112.2408HFIS/05 - ASTRONOMIA E ASTROFISICA