The MBH - Mstar relation of obscured AGNs at high redshift

We report the detection of broad Ha emission in three X-ray selected obscured AGNs at z similar to 1-2. By exploiting the Ha width and the intrinsic X-ray luminosity, we estimate their black hole masses, which are in the range 0.1-3 x 10(9) M-circle dot. By means of multi-band photometric data, we measure the stellar mass of their host galaxy and, therefore, infer their M-BH/M-star ratio. These are the first obscured AGNs at high-z, selected based on their black hole accretion (i.e. on the basis of their X-ray luminosity), that can be located on the M-BH - M-star relation at high-z. All of these obscured high-z AGNs are fully consistent with the local M-BH - M-star relation. This result conflicts with those for other samples of AGNs in the same redshift range, whose M-BH/M-star ratio departs significantly from the value observed in local galaxies. We suggest that the obscured AGNs in our sample are in an advanced evolutionary stage, have already settled onto the local M-BH-M-star relation, and whose nuclear activity has been temporarily revived by recent galaxy interactions.