  Using the KEPLER hydrodynamics code, 464 models of thermonuclear X-ray
bursters were performed across a range of accretion rates and compositions. We
present the library of simulated burst profiles from this sample, and examine
variations in the simulated lightcurve for different model conditions. We find
that the recurrence time varies as a power law against accretion rate, and
measure its slope while mixed H/He burning is occurring for a range of
metallicities, finding the power law gradient to vary from $\eta = 1.1$ to
$1.24$. We also identify the accretion rates at which mixed H/He burning stops
and a transition occurs to different burning regimes. We also explore how
varying the accretion rate and metallicity affects burst morphology in both the
rise and tail.
