  We will present first results of ESO-VLT AO-assisted integral-field
spectroscopy of a sample of X-ray bright AGN with redshifts of 0.04 < z < 1. We
constructed this sample by cross-correlating the SDSS and ROSAT surveys and
utilizing typical AO constraints. This sample allows for a detailed study of
the NIR properties of the nuclear and host environments with high spectral
resolution on the 100 pc scale. These objects can then be compared directly to
the local (z<0.01) galaxy populations (observed without AO) at the same linear
scale. As a current example, we will present observations of the z=0.034
Seyfert 1.8 galaxy Mrk 609 with the new AO-assisted integral-field spectrometer
SINFONI at the VLT. The successful observations show, that in the future -
while having observed more objects - we will be able to determine the presence,
frequency and importance of nuclear bars and/or circum-nuclear star forming
rings in these objects and address the question of how these X-ray luminous AGN
and their hosts are linked to optically/UV-bright QSOs, low-z QSOs/radio
galaxies, or ULIRGs.
