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Table 2:

Parameter values and their 1-$\sigma $ errors for all data groups.
  Group A Group B Group C1 Group C2 Group C3
parameter pers dip pers dip pers dip pers dip pers dip
neutral abs.                    
$N_{\rm H}^a$ $1.28\pm0.05$ $3.81\pm0.8$ $1.10 \pm 0.03$ $2.21\pm 0.17$ $1.11 \pm 0.05$ $2.36 \pm 0.13$ $0.82\pm0.02$ $1.48\pm0.03$ $0.84\pm0.20$ $1.25 \pm 0.03$
CI                    
$N_{\rm H}^a$ $4.05\pm0.25$ $1.8\pm1.6$ $0.95 \pm 0.10$ $5.28\pm0.56$ $3.28_{\rm -0.40}^{+0.18}$ $5.9\pm0.6$ $1.95 \pm 0.07$ $4.1\pm0.1$ $1.09 \pm 0.08$ $3.42\pm0.13$
Tc $66\pm3$ <80 $61\pm4$ $63\pm5$ $70\pm3$ $70\pm7$ $73\pm2$ $69\pm1$ $80\pm4$ $65\pm2$
$\sigma_{v}^b$ <12.27 $ 0. \rm fixed $ <4.83 $123\pm30$ <7.6 <11.1 <4.7 <11.2 <3.57 <15.91
PI                    
$N_{\rm H}^a$ $41\pm4$ $160_{-60}^{\rm +10}$ $37\pm4$ $74\pm11$ $46\pm4$ $140 \pm 10$ $39\pm4$ $80\pm3$ $19\pm2$ $51\pm2$
$\log{\xi} $ $2.35\pm0.04$ $2.24\pm0.04$ $2.56\pm0.04$ $2.36\pm0.05$ $2.40\pm0.04$ $2.39\pm0.03$ $2.63\pm0.04$ $2.38\pm 0.01$ $2.51\pm0.04$ $2.33 \pm 0.02$
$\sigma_{v}^b$ <8.7 <6.1 <32.5 $21\pm9$ <48 $11_{-8}^{\rm +5}$ $17\pm2$ $13.\pm3$ $14\pm2$ $11\pm2$
power law                    
normd $1.07 \pm 0.05$ $1.60\pm0.16$ $1.80\pm0.08$ $1.11\pm0.17$ $1.76\pm0.07$ $1.92\pm0.12$ $1.85\pm0.05$ $1.15 \pm 0.02$ $1.91\pm0.04$ $1.49 \pm 0.04$
$\Gamma$ $1.23 \pm 0.02$ $1.42\pm0.05$ $1.55\pm0.03$ $1.34 \pm 0.08$ $1.42 \pm 0.02$ $1.46 \pm 0.03$ $1.44 \pm 0.01$ $1.24\pm0.02$ $1.47 \pm 0.01$ $1.35 \pm 0.01$
blackbody                    
normd $3.4\pm0.5$ $22_{-20}^{\rm +17}$ $1.20\pm0.13$ $3.6\pm1.0$ $1.8\pm0.4$ $14.\pm6$ $1.10\pm0.12$ $1.95\pm0.25$ $1.10\pm0.09$ $1.88\pm0.21$
Tc $0.10 \pm 0.01$ $0.08\pm0.02$ $0.14 \pm 0.01$ $0.12\pm0.01$ $0.11\pm0.01$ $0.08\pm0.01$ $0.12 \pm 0.02$ $0.11\pm0.01$ $0.12 \pm 0.02$ $0.11 \pm 0.02$
O VII                    
norme $11 \pm 1$ $136_{-40}^{\rm +65}$ $3.3\pm0.9$ $27_{-7}^{\rm +13}$ $9\pm1$ $40\pm8$ $3.6\pm0.4$ $9.6\pm0.8$ $2.9\pm0.4$ $7.6\pm0.7$
FWHMf $0.28 \pm 0.04$ $0.35 \pm 0.06$ <0.5 $0.22_{-0.06}^{\rm +0.28}$ $0.23\pm0.03$ $0.44\pm0.07$ $0.28\pm0.05$ $0.36 \pm 0.05$ $0.24\pm0.06$ <0.5
O VIII                    
norme $2.7\pm0.3$ $16_{-4}^{\rm +14}$ $1.6_{-0.4}^{\rm +1.6}$ $5._{-2}^{\rm +40}$ $2.39_{-0.47}^{\rm +3.74}$ $8.49_{-2.96}^{\rm +67.96}$ $0.51\pm0.16$ $2.32 \pm 0.26$ $0.87\pm0.21$ $1.56\pm0.24$
FWHMf $0.16 \pm 0.04$ $0.34\pm0.09$ $0.07\pm0.07$ <0.11 $0.07\pm0.05$ $0.05 \pm 0.05$ $0.20_{-0.08}^{\rm +0.10}$ $0.10_{-0.02}^{\rm +0.03}$ $0.33\pm0.09$ $0.19\pm0.05$
$\chi^2$/d.o.f. 1.29 1.41 1.42 1.52 1.38 1.50 1.68 1.83 1.59 1.66
Notes:
a Column densities ($N_{\rm H}$) are given in units of 1021 cm-2 for the neutral, collisionally ionised (CI) and photoionised (PI) absorbers.
b The width $\sigma_v$ of the absorption lines is expressed in km s-1.
c Temperatures, T, are in eV for the collisionally ionised gas and in keV for the blackbody.
d The normalisation (norm) of the powerlaw is given in $10^{44} {\rm ~ph~s^{-1}~keV^{-1}}$ at 1 keV. The normalisation of the blackbody is in units of $10^{15} {\rm ~cm^{2}}$.
e The normalisation of the emission lines (OVII and OVIII) are expressed in units of $10^{42} {\rm ~ph~s^{-1}}$.
f The FWHM of the emission lines is in Å.

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