  While the radio-loud, obscured quasars (the radio galaxies) have been known
and studied for decades, new and sensitive X-ray and mid-infrared surveys are
now beginning to reveal large numbers of their radio-quiet counterparts beyond
the local Universe. Consequently, we are approaching the compilation of a
relatively complete census of AGN of all types coving a large fraction of
cosmic time. This is revealing a remarkably intimate connection between the
supermassive black hole and its host galaxy. The workshop reported here was
designed to explore the results of these rapid observational developments and
the nature of the relationships between the stellar and AGN components.
