XMM-Newton observations of two Compton thick candidates

We propose the observation of two Compton thick candidates selected within theextragalactic sources of the Second Palermo BAT Catalogue, according to theirposition in a N_H vs softness ratio (F210 keV/F20100 keV) plot. We aim attheir full spectral characterization through broadband (0.2150 keV) highquality spectroscopy, in order to confirm their Compton thick nature.