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   PR # 41185
   We propose a 100ks ASCA observation of the Seyfert 2 galaxy NGC1068.
   The ASCA PV observation revealed that the soft X-ray emission is
   dominated by starburst emission, and the scattered AGN emission
   appears above 3 keV. The prominent iron K line complex, which consits
   at least 3 components, are emitted from the scattering matter. A
   recent improved analysis shows eveidence for the Compton shoulder at
   the base of 6.4 keV line, which implies the line is scattered by
   Compton-thick cold matter. Contrary to this, the higher energy lines
   are believed to be emitted from warm, optically thin gas. This
   proposed long observation provides precise measurements of the
   Compton shoulder and the other line components to study detailed
   physical condition of the nuclear matter in Seyfert 2 nuclei.
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