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Two brightest cluster galaxies (BCGs), namely Abell 1836-BCG and Abell3565-BCG, were observed with the Advanced Camera for Surveys (ACS) and theSpace Telescope Imaging Spectrograph (STIS) on board the Hubble SpaceTelescope. By modeling the available photometric and kinematic data, itresulted that the mass of Abell 1836-BCG and Abell 3565-BCG areM_bh=4.8(+0.8,-0.7)x10^9 M_sun and M_bh=1.3(+0.3,-0.4)x10^9 M_sun at 1 sigmaconfidence level, respectively.

The Black Hole Mass of Abell 1836-BCG and Abell 3565-BCG