******************************************************
   PR # 41162
   ASCA results obtained for the Seyfert 2 NGC5252 (Cappi et al. 1996b)
   have shown that a flat (2-10 keV) spectrum associated with a weak
   iron line cannot be explained by enhanced reflection because of the
   weak iron line. Therefore, they do not fit easily into simplest
   versions of unified models. We propose to observe the bright Seyfert
   2 NGC 7674 and 1040+706 to investigate this problem. Ginga
   observations indicate that both sources have flat spectra (Gamma(2-10
   keV)=1.4) and low upper limits on their Fe K line. The scientific
   goals of the proposal are: i) to provide tight constraints on the
   absorption, photon index and Fe K line parameters; ii) to test
   unified models based on reflection from neutral matter, and iii) to
   look for and model the soft (E < 2 keV) X-ray emission of these Sey2.
  ******************************************************