*************************************************************************
   52150
   X-ray absorption is common in low luminosity AGN, yet uncommon in
   quasars (only 3 documented cases). New AO4 observations of one of
   these, PG1114+445, show strong X-ray absorption typical of highly
   ionized gas. HST observations show a strong Ovi 1034 absorption line.
   We demonstrate that a good way of detecting warm absorbers is to
   observe objects with strong UV absorption lines. PG1309+355 shows such
   lines and some X-ray absorption in a poorly exposed ROSAT spectrum.
   This is an ideal ASCA target which is likely to show as another high
   luminosity X-ray absorbed AGN. We will study the ionization, column
   density and K-line and edges in this source and will investigate the
   general question of X-ray absorption across a large luminosity range.
 *************************************************************************