TIBURZI, CaterinaCaterinaTIBURZI0000-0002-1110-5882Johnston, S.S.Johnston0000-0001-6651-4811Bailes, M.M.BailesBates, S. D.S. D.Bates0000-0002-8265-4344Bhat, N. D. R.N. D. R.Bhat0000-0001-5902-3731BURGAY, MARTAMARTABURGAYBurke-Spolaor, S.S.Burke-SpolaorChampion, D.D.ChampionCoster, P.P.CosterD'AMICO, NICOLO'NICOLO'D'AMICOKeith, M. J.M. J.KeithKramer, M.M.KramerLevin, L.L.LevinMILIA, SabrinaSabrinaMILIANg, C.C.NgPOSSENTI, ANDREAANDREAPOSSENTIStappers, B. W.B. W.StappersThornton, D.D.Thorntonvan Straten, W.W.van Straten2020-09-252020-09-252017http://hdl.handle.net/20.500.12386/27472We present the polarization analysis of a sample of 49 long-period pulsars, whose spin periods range from a few hundred milliseconds to about two and a half seconds. They were all discovered during the mid-latitude part of the HTRU survey (Keith et al. 2010MNRAS.409..619K; Bates et al. 2012MNRAS.427.1052B) apart from PSR J1846-4249 (that has been discovered in the high latitude survey and it will be presented in one of the next papers of the HTRU series). <P />After discovery and confirmation, the pulsars were followed-up with the third Parkes Digital Filterbank, observing them for at least one year to allow the determination of a complete timing solution. (2 data files).enDatabasehttps://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/436/35572017yCat..74363557TFIS/05 - ASTRONOMIA E ASTROFISICA