\begin{table}%t1
\caption{\label{table1}Properties of the observed \hi~halo clouds.}
\small%\centering
\par
\begin{tabular}{c c c c c c c c c c c c}
\hline\hline
            & \VLSR & $R$ & $z$ & $N_{\rm HI}$ & $s$ &$D$ &\FWHM & $T_{\rm kin}$&     $\langle n \rangle$           &   $P$    &  $M_{\hi}$  \\
             & \kms&kpc &kpc     & \unith &arcmin&pc & \kms   &K       & ${\rm cm^{-3}}$ &  K$~{\rm cm^{-3}}$ &     \msun    \\
\hline 
113.3+27.0  & --40 &10.5 & 1.8 & 16(2) & 13&16(7)& 7.0  & 1080(150) & 0.33(0.15) & 360(170)& 25(22)    \\
113.2+25.5  & --32 &10.0 & 1.4 &  6(1) &  9&8(5) & 4.0  &350(90)  & 0.23(0.14) &  80(50) &  3(4)   \\
116.2+23.6  & --68 &12.5 & 2.8 & 11(2) & 25&51(17)&3.0  &200(70)  & 0.07(0.03) &  14(8)  & 120(80) \\
116.7+22.8  & --81 &14.5 & 3.5 & 25(3) & 27&70(19)&5.1  &570(110) & 0.12(0.04) &  68(26) & 770(440) \\     
116.5+21.4  & --42 &10.5 & 1.5 & 36(4) & 13&14(6) &5.4  &650(120) & 0.70(0.30) & 455(210)&  45(39) \\
115.0+23.9  & --84 &14.5 & 3.9 & 15(3) & 22&60(20)&3.3  & 240(70)  & 0.08(0.03) &  19(7) & 220(140)  \\
115.4+22.4  & --66 &12.0 & 2.5 & 35(3) & 18&34(12)&10.0  &2200(220) & 0.33(0.12) & 730(275)& 260(180)    \\ 
117.3+24.0  & --71 &13.0 & 3.0 & 36(3) & 27&58(18)&8.1  &1440(170) & 0.20(0.06) & 290(90) & 770(490)    \\
118.0+24.6  & --71 &13.0 & 3.1 & 20(3) & 18&40(15)&5.0  &550(110) & 0.16(0.07) &  87(40) & 200(150) \\
118.0+24.0  & --72 &13.0 & 3.0 & 74(4) & 18&40(15)&21.1  &9800(460) & 0.60(0.22) &5800(2140)&750(550)  \\
117.5+25.2  & --74 &13.0 & 3.0 & 60(4) & 18&40(15)& 11.6 &2960(260) & 0.48(0.18) &1449(550) &600(440)  \\
114.5--15.9   & --38 &10.5 &-1.0 &10(2) & 18&18(7) & 4 &350(90)  & 0.18(0.08) &  62(31) &  20(16) \\
113.6--12.4  & --85 &4.5 &-1.9 &  16(2) & 13&35(14)& 4 &350(90)  & 0.14(0.06) &  50(25) & 120(100) \\
113.0--12.4  & --55 &12.0 &-1.2 & 41(3) & 18&28(9) & 6.7 &990(150) & 0.49(0.16) & 470(170)& 205(130) \\ 
113.0--13.0  & --40 &10.5 &-0.9 &  28(3)&  9&9(5) & 4.4  &425(100) & 1.02(0.32) & 435(170)& 14(16) \\
113.3--14.1  & --57 &12.0 &-1.3 & 39(4) &   &&   4.9     &510(100) &            &  &  \\
113.6--13.5  & --50 &11.5 &-1.3 & 68(5) &   &&   7.0     &1080(150) &            &  &    \\ 
114.3+21.8 & --75 &13.5 & 3.0 &  7(-)  &  9&21(12)&    &       &            &  &   \\
128.8--18.5  & --58 &14.0 &-1.9 & 54(6) &   &   & 4.8    &510(100) &            &  &  \\
131.0--19.2  & --72 &15.0 &-2.8 & 49(5) &   &  &  5.4    &640(120) &            &  &  \\
130.6--19.5  & --68 &14.0 &-2.5 & 35(3) &   &  &  6.0    &780(130) &            &  &  \\
112.1+27.3  & --39 &10.5 & 1.8 &  6(1) &  9&10(6) &5.3   &620(120) & 0.20(0.12) & 126(80) & 4(5)  \\
113.8+28.7  & --69 &12.5 & 3.6 &  9(2) & 18&39(14)&6.0  &790(130) & 0.08(0.03) &  61(25) & 90(70) \\ 
112.4+29.9  & --65 &12.5 & 3.7 &  4(1) &  9&20(11)&2.0  &80(40)  & 0.07(0.04) &   6(5) & 11(13)  \\
114.7+29.6  & --89 &15.0 & 5.4 & 19(3) &   &      & 3.6 &285(80)  &            &    &    \\ 
\hline
\end{tabular}
\tablefoot{\VLSR~ is the line of sight
  velocity in \kms, $R$~ is the Galactocentric distance. $z$  is the height
  above mid-plane. $N_{\rm HI}$ is the \hi~column density. $s$ is the measured
  angular diameter. $D$  is the spatial diameter. \FWHM\ is the full width half
  maximum of the line width. $T_{\rm kin}$  the kinetic  temperature. $\langle n \rangle$~ the volume \hi~density. $P$ is the pressure of the \hi~gas. $M_{\hi}$ the visible \hi~mass of the cloud.}
\end{table}