\begin{table}%t2
%\centering
\par
\caption{\label{table:pc_result}The best-fit spectral parameters obtained with the partial-covering absorber model.}
\begin{tabular}{llllllllll}
\hline\hline
\noalign{\smallskip}
System   &   $Z_{\rm{Fe}}$   & $M_{\rm{WD}}$     & $kT_{\rm{s}}$  & $n\rm{H}$\tablefootmark{a}   & $n\rm{H}_{\rm{PC}}$\tablefootmark{b}   & $C_{\rm{PC}}$\tablefootmark{c} & $\chi^2_\nu(\nu)$ & $F_{2,10}$\tablefootmark{d} & $F_{12,40}$\tablefootmark{e} \\
   &   $(Z_\odot)$                    & $(M_\odot)$       &  (keV)         & $10^{22}~\rm{cm}^{-2}$     & $10^{22}~\rm{cm}^{-2}$\\
\hline
FO Aqr & $0.10^{\rm +0.03}_{-0.09}$ & $0.45^{\rm +0.08}_{-0.03}$ & $14.0^{\rm +4.0}_{-1.4}$ & $8.20^{\rm +2.50}_{-2.67}$ & $373^{\rm +133}_{-78}$ &  $0.79^{\rm +0.05}_{-0.16}$& $0.96(386)$ & $4.27$ & $6.00$ \\
  &  &  &  &  & $38.4^{\rm +13.4}_{-7.5}$$^{{\rm f}}$ &  1.0 (fixed) &  &  &  \\
XY Ari & $0.43^{\rm +0.04}_{-0.03}$ & $1.04^{\rm +0.15}_{-0.14}$ & $61.0^{\rm +26.2}_{-16.2}$ & $8.97^{\rm +0.44}_{-0.42}$ & $114^{\rm +34}_{-25}$ &  $0.36^{\rm +0.06}_{-0.04}$& $1.11(457)$ & $1.59$ & $2.73$ \\
MU Cam & $0.59^{\rm +0.08}_{-0.08}$ & $0.95^{\rm +0.36}_{-0.13}$ & $49.9^{\rm +75.6}_{-12.5}$ & $5.05^{\rm +1.07}_{-1.32}$ & $91.0^{\rm +33.2}_{-26.9}$ &  $0.56^{\rm +0.06}_{-0.07}$& $1.02(291)$ & $1.03$ & $1.79$ \\
BG CMi & $0.22^{\rm +0.05}_{-0.05}$ & $1.14^{\rm +0.09}_{-0.17}$ & $76.9^{\rm +20.3}_{-24.7}$ & $4.08^{\rm +3.09}_{-4.08}$ & $25.4^{\rm +10.0}_{-6.7}$ &  $0.53^{\rm +0.23}_{-0.22}$& $0.98(350)$ & $2.24$ & $3.18$ \\
V709 Cas & $0.22^{\rm +0.05}_{-0.04}$ & $1.22^{\rm +0.05}_{-0.20}$ & $94.5^{\rm +15.0}_{-36.2}$ & $1.87^{\rm +0.56}_{-0.65}$ & $90.7^{\rm +31.2}_{-21.3}$ &  $0.38^{\rm +0.03}_{-0.03}$& $0.99(382)$ & $4.12$ & $5.42$ \\
TV Col & $0.49^{\rm +0.06}_{-0.06}$ & $0.91^{\rm +0.14}_{-0.10}$ & $45.7^{\rm +16.6}_{-9.1}$ & $3.38^{\rm +1.30}_{-2.63}$ & $35.2^{\rm +19.6}_{-14.4}$ &  $0.39^{\rm +0.16}_{-0.08}$& $1.08(383)$ & $5.08$ & $5.92$ \\
TX Col & $0.47^{\rm +0.12}_{-0.12}$ & $0.82^{\rm +0.24}_{-0.16}$ & $37.4^{\rm +26.3}_{-11.8}$ & $1.56^{\rm +1.67}_{-1.56}$ & $32.9^{\rm +27.8}_{-15.7}$ &  $0.38^{\rm +0.13}_{-0.13}$& $1.18(341)$ & $1.23$ & $1.18$ \\
YY Dra & $0.50^{\rm +0.19}_{-0.11}$ & $0.67^{\rm +0.30}_{-0.14}$ & $26.3^{\rm +25.9}_{-8.3}$ & $0.47^{\rm +1.12}_{-0.47}$ & $90.7^{\rm +77.5}_{-72.3}$ &  $0.32^{\rm +0.20}_{-0.26}$& $1.07(340)$ & $3.77$ & $2.74$ \\
PQ Gem & $0.24^{\rm +0.05}_{-0.05}$ & $1.15^{\rm +0.10}_{-0.18}$ & $78.8^{\rm +24.2}_{-26.6}$ & $1.94^{\rm +1.60}_{-1.94}$ & $38.0^{\rm +28.8}_{-14.2}$ &  $0.41^{\rm +0.12}_{-0.10}$& $1.17(386)$ & $2.49$ & $3.11$ \\
EX Hya & $0.56^{\rm +0.04}_{-0.03}$ & $0.42^{\rm +0.02}_{-0.02}$ & $12.7^{\rm +0.9}_{-0.9}$ & $0.69^{\rm +0.23}_{-0.20}$ & $101^{\rm +13}_{-12}$ &  $0.42^{\rm +0.05}_{-0.04}$& $1.22(358)$ & $9.10$ & $3.56$ \\
NY Lup & $0.55^{\rm +0.04}_{-0.04}$ & $1.15^{\rm +0.08}_{-0.07}$ & $78.8^{\rm +18.4}_{-12.0}$ & $6.13^{\rm +0.60}_{-0.63}$ & $145^{\rm +31}_{-22}$ &  $0.46^{\rm +0.02}_{-0.02}$& $1.19(307)$ & $3.29$ & $6.03$ \\
V2400 Oph & $0.25^{\rm +0.02}_{-0.04}$ & $0.62^{\rm +0.06}_{-0.05}$ & $23.1^{\rm +3.8}_{-2.9}$ & $1.69^{\rm +0.89}_{-1.69}$ & $308^{\rm +40}_{-26}$ &  $0.60^{\rm +0.07}_{-0.09}$& $1.12(457)$ & $5.00$ & $5.99$ \\
  &  &  &  &  & $38.3^{\rm +18.7}_{-15.0}$$^{{\rm f}}$ &  1.0 (fixed) &  &  &  \\
AO Psc & $0.44^{\rm +0.08}_{-0.04}$ & $0.61^{\rm +0.08}_{-0.04}$ & $22.5^{\rm +5.1}_{-2.3}$ & $4.99^{\rm +0.86}_{-2.41}$ & $54.4^{\rm +23.4}_{-29.7}$ &  $0.38^{\rm +0.08}_{-0.07}$& $1.03(595)$ & $4.96$ & $4.06$ \\
V1223 Sgr & $0.29^{\rm +0.03}_{-0.02}$ & $0.75^{\rm +0.05}_{-0.05}$ & $31.9^{\rm +3.9}_{-3.6}$ & $9.45^{\rm +0.85}_{-0.84}$ & $219^{\rm +29.7}_{-25.7}$ &  $0.50^{\rm +0.04}_{-0.02}$& $1.19(333)$ & $9.52$ & $15.57$ \\
RX J2133 & $0.38^{\rm +0.04}_{-0.06}$ & $0.91^{\rm +0.19}_{-0.17}$ & $45.7^{\rm +24.2}_{-14.6}$ & $9.33^{\rm +1.39}_{-1.04}$ & $275^{\rm +63.3}_{-39.7}$ &  $0.58^{\rm +0.08}_{-0.06}$& $1.16(331)$ & $2.10$ & $4.64$ \\
IGR J17303 & $0.29^{\rm +0.05}_{-0.05}$ & $1.06^{\rm +0.19}_{-0.14}$ & $63.8^{\rm +39.2}_{-17.0}$ & $4.54^{\rm +0.61}_{-0.66}$ & $240^{\rm +37.0}_{-26.6}$ &  $0.69^{\rm +0.03}_{-0.03}$& $1.08(364)$ & $2.07$ & $5.60$ \\
IGR J17195 & $0.38^{\rm +0.05}_{-0.05}$ & $1.03^{\rm +0.24}_{-0.22}$ & $59.6^{\rm +49.9}_{-23.0}$ & $1.99^{\rm +0.54}_{-1.06}$ & $79.6^{\rm +47.3}_{-29.0}$ &  $0.36^{\rm +0.10}_{-0.04}$& $0.95(373)$ & $3.99$ & $4.96$ \\
\hline
\end{tabular}
\tablefoot{The errors are at 90\% confidence levels.
\tablefoottext{a}{The absorption column density of fully-covering absorbent.}
\tablefoottext{b}{The absorption column density of the partial-covering absorbent (see text).}
\tablefoottext{c}{The partial-covering fraction.} 
\tablefoottext{d}{$2{-}10$~keV flux in units of $10^{-11}~\ergcms$.}
\tablefoottext{e}{$12{-}40$~keV flux in units of $10^{-11}~\ergcms$.}
\tablefoottext{f}{The column density of the additional absorbed component (see text).}}\vspace*{1.5mm}
\end{table}