Reverberation Mapping of High-z, High-luminosity Quasars
  We present Reverberation Mapping results after monitoring a sample of 17
high-z, high-luminosity quasars for more than 10 years using photometric and
spectroscopic capabilities. Continuum and line emission flux variability is
observed in all quasars. Using cross-correlation analysis we successfully
determine lags between the variations in the continuum and broad emission lines
for several sources. Here we present a highlight of our results and the
determined radius--luminosity relations for Ly_alpha and CIV.
