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Table 10:

Median and standard deviation properties for the final compilation of our LINER sample in X-rays.
Chandra XMM-Newton Total AGN Non-AGN K-S prob.$^{(\ast)}$
  (1) (2) (3) (4) (5) (6)
$\Gamma$ 2.05 ${\pm}$ 0.42 1.99 ${\pm}$ 0.37 _totmedian 2.02 ${\pm}$ 0.48 2.43 ${\pm}$ 0.57 66%
T (keV) 0.57 ${\pm}$ 0.22 0.61 ${\pm}$ 0.38 0.54 ${\pm}$ 0.30 0.58 ${\pm}$ 0.30 0.35 ${\pm}$ 0.27 61%
${\log({\rm NH1})}$ 21.45 ${\pm}$ 0.14 21.00 ${\pm}$ 0.74 21.32 ${\pm}$ 0.71 21.32 ${\pm}$ 0.71 21.43 ${\pm}$ 0.71 99%
${\log({\rm NH2})}$ 21.93 ${\pm}$ 1.02 21.94 ${\pm}$ 1.23 $21.93\pm1.36$ \begin{center}\vbox{\input{NH2_totmedianAGN}
}\end{center} \begin{center}\vbox{\input{NH2_totmedianSB}
}\end{center} 2%
$\log(L(0.5\hbox{--}2~{\rm
keV}))$ 39.95 ${\pm}$ 1.19 \begin{center}\vbox{\input{XMMmeanlums}
}\end{center} \begin{center}\vbox{\input{lums_totmedian}
}\end{center} \begin{center}\vbox{\input{lums_totmedianAGN}
}\end{center} \begin{center}\vbox{\input{lums_totmedianSB}
}\end{center} 21%
$\log(L(2\hbox{--}10~{\rm
keV}))$ 39.85 ${\pm}$ 1.17 \begin{center}\vbox{\input{XMMmeanlumh}
}\end{center} _totmedian \begin{center}\vbox{\input{lumh_totmedianAGN}
}\end{center} \begin{center}\vbox{\input{lumh_totmedianSB}
}\end{center} 29%
EW (eV) 164 ${\pm}$ 160 144 ${\pm}$ 213 211 ${\pm}$ 214 144 ${\pm}$ 167 296 ${\pm}$ 442  

$^{(\ast)}$Kolmogorov-Smirnov test probability that the two distributions arise from the same parent distribution.


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