Morabito, L. K.L. K.MorabitoMatthews, J. H.J. H.MatthewsBest, P. N.P. N.BestGürkan, G.G.GürkanJarvis, M. J.M. J.JarvisPRANDONI, ISABELLAISABELLAPRANDONIDuncan, K. J.K. J.DuncanHardcastle, M. J.M. J.HardcastleKunert-Bajraszewska, M.M.Kunert-BajraszewskaMechev, A. P.A. P.MechevMooney, S.S.MooneySabater, J.J.SabaterRöttgering, H. J. A.H. J. A.RöttgeringShimwell, T. W.T. W.ShimwellSmith, D. J. B.D. J. B.SmithTasse, C.C.TasseWilliams, W. L.W. L.Williams2022-02-252022-02-2520200004-6361http://hdl.handle.net/20.500.12386/31487We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from observed flux densities, the wrong sign convention was used. This resulted in an underestimation of the radio powers by a median value of 0.6 dex and a maximum of 1 dex. The conclusions of the paper are unchanged.STAMPAen10.1051/0004-6361/201833821e2-s2.0-85089942389https://www.aanda.org/articles/aa/full_html/2020/08/aa33821e-18/aa33821e-18.htmlhttps://api.elsevier.com/content/abstract/scopus_id/850899423892020A&A...640C...4MFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering