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A simple regression analysis designed for predicting the supermassive blackhole mass from the effective radius and mean effective surface brightness ofthe host bulge has been performed using the data from Barway & Kembhavi(arXiv:0705.1508). The scatter in the log M_bh direction is 0.32 dex, greaterthan reported and comparable with values obtained using a single predictorquantity such as luminosity, velocity dispersion or Sersic index.

Comment on: A SuperMassive Black Hole Fundamental Plane for Ellipticals