Treu, T.T.Treu0000-0001-9261-7849Brammer, G.G.BrammerDiego, J. M.J. M.DiegoGrillo, C.C.GrilloKelly, P. L.P. L.KellyOguri, M.M.OguriRodney, S. A.S. A.RodneyRosati, P.P.RosatiSharon, K.K.SharonZitrin, A.A.ZitrinBalestra, I.I.BalestraBradac, M.M.BradacBroadhurst, T.T.BroadhurstCaminha, G. B.G. B.CaminhaHalkola, A.A.HalkolaHoag, A.A.HoagIshigaki, M.M.IshigakiJohnson, T. L.T. L.JohnsonKarman, W.W.KarmanKawamata, R.R.KawamataMERCURIO, AMATAAMATAMERCURIOSchmidt, K. B.K. B.SchmidtStrolger, L. -G.L. -G.StrolgerSuyu, S. H.S. H.SuyuFilippenko, A. V.A. V.FilippenkoFoley, R. J.R. J.FoleyJha, S. W.S. W.JhaPatel, B.B.Patel2020-07-022020-07-022016http://hdl.handle.net/20.500.12386/26283Since the discovery of SN Refsdal on 2014 November 11, the MACSJ1149.5+2223 field has been observed in great detail, with HST imaging in optical and infrared bands, and deep spectroscopy from HST, Keck, and the VLT. <P />The HST grism spectroscopy comprises two data sets. The GLASS data consist of 10 orbits of exposures taken through the G102 grism and 4 orbits of exposures taken through the G141 grism, spanning the wavelength range 0.81-1.69um. The GLASS data were taken at two approximately orthogonal position angles (PAs) to mitigate contamination by nearby sources (the first one on 2014 February 23-25, the second PA on 2014 November 3-11). The SN Refsdal follow-up spectra were taken between 2014 December 23 and 2015 January 4. For more details the reader is referred to Schmidt et al. (2014ApJ...782L..36S) and Treu et al. (2015, J/ApJ/812/114) for GLASS, and G. B. Brammer et al. (2015, in preparation) and P. L. Kelly et al. (2015, in preparation) for the deeper follow-up data. <P />Integral-field spectroscopy was obtained with the MUSE instrument on the VLT between 2015 February 14 and 2015 April 12, as part of a Director Discretionary Time program to observe SN Refsdal (PI Grillo). Details of the data acquisition and processing are given in a separate paper (Grillo et al. 2015, arXiv:1511.04093). Spectroscopy of the field was obtained using the DEIMOS spectrograph on the 10m Keck II telescope on 2014 December 20. (3 data files).enDatabase10.26093/cds/vizier.18170060http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJ/817/602016yCat..18170060TFIS/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