\begin{table}%t3
%\centering
\par
\caption{\label{table:mwd_compare}Estimated WD masses compared with previous reports in the X-ray band.}
\begin{tabular}{lllllllll}
\hline\hline
\noalign{\smallskip}
System   & {\it Suzaku}\tablefootmark{a}         & {\it Swift}\tablefootmark{b}   & {\it RXTE}\tablefootmark{c}    & {\it RXTE}\tablefootmark{d}             & {\it Ginga}\tablefootmark{e}           & {\it ASCA}\tablefootmark{f} \\
& XIS+HXD              & BAT           & PCA+HEXTE     & PCA                    & LAC   & SIS\\
& $M_{\rm{WD}}$        & $M_{\rm{WD}}$ & $M_{\rm{WD}}$ & $M_{\rm{WD}}$          & $M_{\rm{WD}}$      & $M_{\rm{WD}}$\\
\hline
FO Aqr &  $0.45^{\rm +0.08}_{-0.03}$  & $0.61\pm0.05$ & $0.60\pm0.05$ & $0.88^{\rm +0.07}_{-0.09}$ & $0.92^{\rm +0.30}_{-0.34}$ & $1.05({>}0.44)$\\
XY Ari &  $1.04^{\rm +0.15}_{-0.14}$  & $0.96\pm0.12$ &             & $0.97^{\rm +0.16}_{-0.17}$ &                      & \\
MU Cam &  $0.95^{\rm +0.36}_{-0.13}$  & $0.74\pm0.13$ &             &                      &                      & \\
BG CMi &  $1.14^{\rm +0.09}_{-0.17}$  & $0.67\pm0.19$ & $0.85\pm0.12$ & $1.15^{\rm +0.06}_{-0.06}$ & $1.09({>}0.94)$          & \\
V709 Cas &  $1.22^{\rm +0.05}_{-0.20}$  & $0.96\pm0.05$ & $0.90\pm0.10$ & $1.08^{\rm +0.05}_{-0.17}$ &                    & \\
TV Col &  $0.91^{\rm +0.14}_{-0.10}$  & $0.78\pm0.06$ & $0.84\pm0.06$ & $0.97^{\rm +0.02}_{-0.05}$ & $1.3({>}0.9)$            & $0.51^{\rm +0.41}_{-0.22}$\\
TX Col &  $0.82^{\rm +0.24}_{-0.16}$  & $0.67\pm0.10$ & $0.70\pm0.30$ & $0.74^{\rm +0.05}_{-0.05}$ & $0.48^{\rm +0.06}_{-0.09}$ & $0.66^{\rm +0.73}_{-0.42}$\\
YY Dra &  $0.67^{\rm +0.30}_{-0.14}$  & $0.50\pm0.11$ & $0.75\pm0.05$ &                      &                      & \\
PQ Gem &  $1.15^{\rm +0.10}_{-0.18}$  & $0.65\pm0.09$ & $0.65\pm0.20$ &                     & $1.29({>}1.17)$          & \\
EX Hya &  $0.42^{\rm +0.02}_{-0.02}$  & $0.66\pm0.17$ & $0.50\pm0.05$ & $0.44^{\rm +0.03}_{-0.03}$ & $0.46^{\rm +0.04}_{-0.04}$ & $0.48^{\rm +0.10}_{-0.06}$\\
NY Lup &  $1.15^{\rm +0.08}_{-0.07}$  & $1.09\pm0.07$ &           &                      &                     & \\
V2400 Oph &  $0.62^{\rm +0.06}_{-0.05}$  & $0.81\pm0.10$ & $0.59\pm0.05$ & $0.71^{\rm +0.07}_{-0.03}$ &  & $0.68^{\rm +0.42}_{-0.24}$ \\
AO Psc &  $0.61^{\rm +0.08}_{-0.04}$  & $0.55\pm0.06$ & $0.65\pm0.05$ & $0.60^{\rm +0.03}_{-0.03}$ & $0.56^{\rm +0.16}_{-0.20}$ & $0.40^{\rm +0.13}_{-0.10}$\\
V1223 Sgr &  $0.75^{\rm +0.05}_{-0.05}$  & $0.65\pm0.04$ & $0.95\pm0.05$ & $1.07^{\rm +0.08}_{-0.09}$ &                   & $1.28({>}0.84)$\\
RX J2133 &  $0.91^{\rm +0.19}_{-0.17}$  & $0.91\pm0.06$ &           &                      &                      & \\
IGR J17303 &  $1.06^{\rm +0.19}_{-0.14}$  & $1.08\pm0.07$ &         &                      &                      & \\
\hline
\end{tabular}
\tablefoot{The mass ranges associated are all 90\% confidence intervals.
\tablefoottext{a}{This work.}
\tablefoottext{b}{\citet{brunschweigeretal2009}.}
\tablefoottext{c}{\citet{suleimanovetal2005}.}
\tablefoottext{d}{\citet{ramsay2000}.}
\tablefoottext{e}{\citet{cropperetal1999}.}
\tablefoottext{f}{\citet{ezukaishida1999}.}}
\end{table}