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   81716
   NGC4395 has been known as the least luminous Seyfert galaxy to date. A
   half-day ASCA observation of this galaxy revealed its highly variable
   X-ray nature in contrast to the other low luminosity active galaxies.
   It suggests an intermediate black hole mass of the order of 10,000 Msun
   and thus a scaled-down version of higher luminosity Seyfert nuclei. The
   X-ray spectrum shows strong evidence for an warm absorber and a Fe K
   line, and a very clear change in the warm absorber has been found in
   response to the continuum flaring. Here, we propose a week-long
   observation of NGC4395 to cover the interesting frequency range of the
   power spectrum, and to investigate the iron K line profile and the
   variable warm absorber.
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