087102

Recent observations point out that Low-luminosity active galactic nuclei comma such LINERs and low power Seyfert galaxies comma might have a different torus configuration compared to more powerful AGNs. The shape of the Compton hump observed above 10 KeV is an excellent tool to study the geometry and the physical features of the reflector. The purpose of this proposal is study a low powered openParL-LEdd sim 10elev-5closePar Seyfert galaxy NGC 5033 comma to study the characteristics of the material surrounding the SMBH. We ask for observations with NuSTAR and XMM-Newton to study the relation between the accretion rate and properties of the reflector openPartorus covering fraction and column densityclosePar and to compare with existing comma similar quality data of a LINER with equal black hole mass and accretion rate.