  How to calculate the gravitational waves (GWs) of
Extreme-mass-ratio-inspirals (EMRIs) in a highly accurate and efficient way
still keeps a challenge. In this paper, we present a so-called fully
recalibrated waveforms for EMRIs with high accuracy. Based on the numerical
data by solving the Teukolsky equations, we recalibrate all mass-ratio
independent coefficients of the factorized waveforms which are used in the
effective-one-body (EOB) models. Due to these new coefficients, the precision
of waveforms is improved enormously, and is much higher than the original forms
and at the same time higher than other existing calibration models. We believe
our model will play an important role in the waveform-template construction of
the space-based GW detectors.
