\begin{table}%t4
\caption{\label{tab:lcfit}Results of the light curve modelling process. }
\par
%\centerline
 {\begin{tabular}{lccc}
\hline\hline
Quantity                      & Value           & Formal          & Adopted         \\
\                             &                 & uncertainty     & uncertainty     \\
\hline
Reference time (HJD)          & 2454821.68051   & 0.00002         & 0.0002          \\
Orbital period (d)            & 0.18591324      &         \mc{(fixed)}              \\
Orbital inclination ($^\circ$)& 81.3            & 0.8             & 2.0             \\
Mass ratio                    & 0.51            & 0.04            & 0.08            \\
Disc radius ($a$)             & 0.189           & 0.015           & 0.05            \\
White dwarf radius ($a$)      & 0.0110          & 0.0013          & 0.003           \\
Secondary star radius ($a$)   & 0.322           & 0.006           & 0.010           \\
\hline \end{tabular}}
\par
\smallskip
 The
formal uncertainties come from the MCMC analysis and the adoped uncertainties
are increased to account for several additional sources of uncertainty. Several
parameters are given in units of $a$, the \reff{orbital} semimajor axis.\end{table}