\begin{table}%t3
\par
\caption{\label{table:3}\texttt{absori} model fits to the X-ray spectra for a sample of 39 BALQSOs with the best statistics.} 
%\centering
\par
\begin{tabular}{ c c c c c} 
\hline\hline 
\noalign{\smallskip}
Name$^{(1)}$ & $\Gamma$$^{(2)}$ & BAL type$^{(3)}$& $\xi$$^{(4)}$ & $N_{\rm{H}}$$^{(5)}$  \\ 
\hline  
J004338.10+004615.9& 1.77 & Lo & $\rm 450^{+300}_{-300 }$ & $\rm 1.05^{+0.40}_{-0.40}$ \\ 
J004341.24+005253.3 & 1.89 & Lo & $\rm 150^{+100}_{-100 }$ & $\rm 6.02^{+1.69}_{-1.69}$ \\ 
B004751.94-523127.9 & 2.32 & Hi & $\rm 450^{+250}_{-250 }$ & $\rm 34.97^{+4.00}_{-4.00}$ \\ 
J010328.7-064633 & 2.17 & Hi & $\rm 150^{+120}_{-120 }$ & $\rm 1.15^{+0.25}_{-0.25}$ \\ 
J023148.80-073906.3 & 2.08 & Hi & $\rm 300^{+200}_{-200 }$ & $\rm 3.93^{+0.88}_{-0.88}$ \\ 
J023224.87-071910.5 & 1.65 & Hi & $\rm 300^{+200}_{-200 }$ & $\rm 7.75^{+3.25}_{-3.25}$ \\ 
J024304.68+000005.4 & 1.73 & Hi & $\rm 205^{+195}_{-195 }$ & $\rm 11.65^{+3.16}_{-3.16}$ \\ 
J030222.08+000631.0 & 1.71 & H & $\rm 100^{+25}_{-25 }$ & $\rm 7.12^{+0.35}_{-0.35}$ \\ 
J07598+6508 & 2.72 & Lo & $\rm 500^{+300}_{-300}$ & $\rm 0.80^{+0.10}_{-0.10}$ \\ 
J084840.5+445732 & 2.03 & Hi & $\rm 500^{+300}_{-300 }$ & $\rm 15.94^{+3.15}_{-3.15}$ \\ 
J085551.24+375752.2 & 1.60 & Hi & $\rm 100^{+50}_{-50 }$ & $\rm 1.06^{+1.00}_{-1.00}$ \\ 
J091127.61+055054.1 & 1.62 & H & $\rm 275^{+125}_{-125 }$ & $\rm 9.50^{+1.50}_{-1.50}$ \\ 
J092104.36+302030.3 & 2.02 & H & $\rm 100^{+100}_{-100 }$ & $\rm 3.5^{+1.0}_{-1.0}$ \\ 
J092238.43+512121.2 & 2.18 & Lo & $\rm 500^{+200}_{-200 }$ & $\rm 0.90^{+0.39}_{-0.39}$ \\ 
J100116.78+014053.5 & 1.90 & Hi & 50 & $\rm 0.17^{+0.05}_{-0.05}$ \\ 
J100120.84+555349.5 & 2.11 & Lo & $\rm 600^{+100}_{-100 }$ & $\rm 0.50^{+0.15}_{-0.15}$ \\ 
 1004+130           & 1.40 & Hi & $\rm 225^{+75}_{-75 }$ & $\rm 0.74^{+0.12}_{-0.12}$ \\ 
J100728.69+534326.7 & 1.85 & nHi & $\rm 425^{+125}_{-125 }$ & $\rm 14.31^{+1.92}_{-1.92}$ \\ 
J101144.33+554103.1 & 1.18 & H & $\rm 100^{+50}_{-50 }$ & $\rm 2.10^{+0.40}_{-0.40}$ \\ 
J102117.74+131545.9 & 2.07 & Lo & $\rm 75^{+25}_{-25 }$ & $\rm 0.60^{+0.10}_{-0.10}$ \\ 
J105154+572408 & 2.18 & Hi & $\rm 50^{+10}_{-10}$ & $\rm 7.40^{+0.50}_{-0.50}$ \\ 
J105201.35+441419.8 & 1.81 & Hi & $\rm 650^{+150}_{-150 }$ & $\rm 36.15^{+3.75}_{-3.75}$ \\ 
J105207.7+573842 & 1.74 & Hi & 50 & 0.86 \\ 
 1115+080      & 1.87 & Hi & $\rm 10^{+7.7}_{-13 }$ & $\rm 1.05^{+1.05}_{-1.05}$ \\ 
J112020.96+432545.1 & 1.56 & H & $\rm 75^{+25}_{-25 }$ & $\rm 0.98^{+0.18}_{-0.18}$ \\ 
J114636.88+472313.3 & 2.02 & Lo & $\rm 110^{+90}_{-90 }$ & $\rm 2.95^{+0.41}_{-0.41}$ \\ 
J120522.18+443140.4 & 1.42 & Hi & $\rm 350^{+50}_{-50 }$ & $\rm 6.72^{+0.42}_{-0.42}$ \\ 
J122307.52+103448.2 & 2.18 & H & $\rm 200^{+50}_{-50 }$ & $\rm 2.65^{+0.25}_{-0.25}$ \\ 
J124520.72-002128.2 & 1.86 & H & 100& 7.90\\ 
1246-057 & 1.61 & Hi & $\rm 400^{+200}_{-200 }$ & $\rm 7.17^{+1.08}_{-1.08}$ \\ 
J132330.44+545955.6 & 1.61 & Hi & $\rm 150^{+150}_{-150 }$ & $\rm 3.65^{+1.35}_{-1.35}$ \\ 
J133553.61+514744.1 & 2.04 & Lo & $\rm 250^{+150}_{-150 }$ & $\rm 5.20^{+1.62}_{-1.62}$ \\ 
J142539.38+375736.7 & 2.53 & Hi & $\rm 100^{+50}_{-50 }$ & $\rm 5.95^{+0.45}_{-0.45}$ \\ 
J143513.89+484149.3 & 1.58 & Hi & $\rm 100^{+50}_{-50 }$ & $\rm 1.45^{+1.00}_{-1.00}$ \\ 
J144727.49+403206.3 & 2.16 & Lo & $\rm 125^{+75}_{-75 }$ & $\rm 0.45^{+0.05}_{-0.05}$ \\ 
J152553.89+513649.1 & 1.83 & Hi & $\rm 375^{+175}_{-175 }$ & $\rm 8.20^{+1.35}_{-1.35}$ \\ 
J154359.44+535903.2 & 1.71 & Hi & $\rm 300^{+300}_{-300 }$ & $\rm 4.42^{+1.37}_{-1.37}$ \\ 
2111-4335 & 1.81 &  Hi & $\rm 100^{+50}_{-50 }$ & $\rm 8.00^{+1.52}_{-1.52}$ \\ 
J213023.61+122252.2 & 1.98 & nH & 10 & $\rm 0.97^{+0.97}_{-1.23}$ \\ 
\hline 
\end{tabular}
\tablefoot {Column~(1): source name; Col.~(2): photon Index (fixed), taken from the absorbed power-law model fits; Col.~(3): the BALQSO subclassification; Col.~(4): ionisation parameter in erg cm s$^{-1}$; Col.~(5): hydrogen column density of absorber in units of $10^{22}$~cm$^{-2}$.}
\end{table}