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Table 3:

absori model fits to the X-ray spectra for a sample of 39 BALQSOs with the best statistics.

Name(1) 		$\Gamma $(2) BAL type(3) $\xi $(4) $N_{\rm {H}}$(5)
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 $\rm 500^{+300}_{-300}$ $\rm0.80^{+0.10}_{-0.10}$
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 $\rm 500^{+200}_{-200 }$ $\rm0.90^{+0.39}_{-0.39}$
J100116.78+014053.5 1.90 Hi 50 $\rm0.17^{+0.05}_{-0.05}$
J100120.84+555349.5 2.11 Lo $\rm 600^{+100}_{-100 }$ $\rm0.50^{+0.15}_{-0.15}$
1004+130 1.40 Hi $\rm 225^{+75}_{-75 }$ $\rm0.74^{+0.12}_{-0.12}$
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 $\rm 75^{+25}_{-25 }$ $\rm0.60^{+0.10}_{-0.10}$
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 $\rm 75^{+25}_{-25 }$ $\rm0.98^{+0.18}_{-0.18}$
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 $\rm 125^{+75}_{-75 }$ $\rm0.45^{+0.05}_{-0.05}$
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 $\rm0.97^{+0.97}_{-1.23}$

Notes. 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 1022 cm-2.


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