089068

We propose simultaneous NuSTAR openPar80 ksecclosePar and XMM-Newton openPar60 ksecclosePar observations of IRASF05054+1718 comma a local openParz = 0.0175closePar Seyfert 2 galaxy comma which hosts a powerful disk wind and where there is evidence of quenching of star formation. In this source comma Swift data suggested the presence of a powerful and high-velocity openParvout aquestionMarkquestionMark 0.1 cclosePar wind comma most likely launched within 100Rg . A short NuSTAR observation confirms the presence of such a wind comma but with a much higher velocity openParvout aquestionMarkquestionMark 0.2 cclosePar. Neither of the two previous observations have the statistical quality needed to fully investigate the physical properties of this wind. Our aim here is to confirm the disk wind at a higher statistical significance.