OLMI, LUCALUCAOLMI0000-0002-9120-5890Cunningham, M.M.Cunningham0000-0002-1162-7947ELIA, Davide QuintinoDavide QuintinoELIAJones, P.P.Jones2020-07-092020-07-092016http://hdl.handle.net/20.500.12386/26397The files are the Mopra telescope data cubes used to produce the channel maps shown in Appendix A. Intensity units are Ta*[K]. Data cubes are not (baseline) reduced. Noise in the maps is not uniform. Frequency resolution is 33.7kHz. (2 data files).enDatabase10.26093/cds/vizier.35940058http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/594/A582016yCat..35940058OFIS/05 - ASTRONOMIA E ASTROFISICA