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   PR # 42130
   We propose a simultaneous Asca / XTE / OSSE observation of a Seyfert
   2 galaxy NGC 4945. This object, already detected by OSSE, is probably
   the brightest Seyfert 2 in hard X-rays. Since its primary component
   is bright yet heavily absorbed, NGC 4945 is the best candidate to
   detect the scattered fraction of the primary X-ray continuum by the
   same medium (most likely the hot electrons) that are likely to be
   responsible for the scattered broad-line flux (visible only in in
   polarized light), and will alow a measurement of the conditions of
   this medium, and in verification of the Seyfert Unified Schemes.
   Since the primary continuum is probably variable, even though this
   object was already observed by Asca, a reobservation is required to
   measure the primary - to - scattered X-ray ratio.
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