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   PR # 42127
   A previous ASCA observation of the Seyfert galaxy NGC 7314 revealed
   an X-ray continuum rapidly variable on a timescale of thousands of
   seconds and an averaged iron K alpha line profile showing complexity
   indicative of relativistic broadening. The response of the line to
   the continuum on these timescales was measured for the first time in
   any AGN and it was shown that the red wing of the line responds to
   the continuum faster than line core. >From this a crude estimate of
   the putative black hole mass was possible. We propose another
   observation to confirm the result with higher significance,
   investigate long-term behavior of the line, and to set even more
   stringent constraints on the structure and physics of the active
   nucleus.
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