Ursini, FrancescoFrancescoUrsiniPetrucci, P. -O.P. -O.PetrucciMatt, G.G.MattBIANCHI, SIMONESIMONEBIANCHICAPPI, MASSIMOMASSIMOCAPPIDADINA, MAUROMAURODADINAGRANDI, PAOLAPAOLAGRANDITORRESI, ELEONORAELEONORATORRESIBallantyne, D. R.D. R.BallantyneDe Marco, B.B.De MarcoDE ROSA, ADRIANO GIUSEPPEADRIANO GIUSEPPEDE ROSAGIROLETTI, MARCELLOMARCELLOGIROLETTIMalzac, J.J.MalzacMarinucci, A.A.MarinucciMiddei, R.R.MiddeiPONTI, GABRIELEGABRIELEPONTITORTOSA, ALESSIAALESSIATORTOSA2021-01-082021-01-0820180035-8711http://hdl.handle.net/20.500.12386/29605We present the analysis of five joint XMM-Newton/NuSTAR observations, 20 ks each and separated by 12 days, of the broad-line radio galaxy 3C 382. The data were obtained as part of a campaign performed in September-October 2016 simultaneously with Very Long Baseline Array. The radio data and their relation with the X-ray ones will be discussed in a following paper. The source exhibits a moderate flux variability in the UV/X-ray bands, and a limited spectral variability especially in the soft X-ray band. In agreement with past observations, we find the presence of a warm absorber, an iron Kα line with no associated Compton reflection hump, and a variable soft excess well described by a thermal Comptonization component. The data are consistent with a `two-corona' scenario, in which the UV emission and soft excess are produced by a warm (kT ≃ 0.6 keV), optically thick (τ ≃ 20) corona consistent with being a slab fully covering a nearly passive accretion disc, while the hard X-ray emission is due to a hot corona intercepting roughly 10 per cent of the soft emission. These results are remarkably similar to those generally found in radio-quiet Seyferts, thus suggesting a common accretion mechanism.STAMPAenArticle10.1093/mnras/sty12582-s2.0-85052466594000439547400092https://academic.oup.com/mnras/article-abstract/478/2/2663/4996367https://academic.oup.com/mnras/pdf-lookup/doi/10.1093/mnras/sty12582018MNRAS.478.2663UFIS/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::PE9_6 Stars and stellar systems