\begin{table} %t2
 \caption{\label{igr112:tab:specfits}Spectral fit results.} 	
 \small%\centerline
{
 \begin{tabular}{lllrr} 
 \hline 
 \hline 
 \noalign{\smallskip} 
 Spectrum$^{{a}}$ & $N_{\rm H}$           & $\Gamma$              & $\chi^2$ (d.o.f.)/ & 	$L_{1 - 10 {\rm ~keV}}$$^{{b}}$\\ 
 		& (10$^{22}$ cm$^{-2}$)	         & 	                  & C-stat (\%)$^{c}$  &    (erg s$^{-1}$) 	     \\
 \hline 
 \noalign{\smallskip} 
001 (2006)	   &	$0.88_{\rm -0.62}^{+0.96}$	&	$\rm 1.89_{\rm -0.92}^{+1.07}$	  & 167.7 (65.8\%)  &$2.35\times10^{-1}$     \\
001--005   &	$2.28_{\rm -1.50}^{+2.21}$	&	$1.34_{\rm -0.96}^{+1.11}$	  & 225.9 (65.8\%)  &$4.32\times10^{-2}$     \\
006	   &	$1.04_{\rm -0.20}^{+0.25}$	&	$1.00_{\rm -0.14}^{+0.16}$	  &1.04 (83)  	    &$4.78$     \\
006 Flare 1&	$0.85_{\rm -0.32}^{+0.46}$	&	$0.94_{\rm -0.28}^{+0.31}$	  &0.66 (17) 	    &$8.68$      \\
006 Flare 2&	$1.11_{\rm -0.49}^{+0.79}$	&	$0.91_{\rm -0.32}^{+0.42}$	  &1.16 (25)	    &$8.32$      \\
006 Flare 3&	$0.83_{\rm -0.42}^{+0.62}$	&	$0.82_{\rm -0.40}^{+0.44}$	  &0.93 (10)	    &$11.1$      \\
006 Flare 4&	$0.88_{\rm -0.31}^{+0.38}$	&	$1.03_{\rm -0.31}^{+0.32}$	  &623.6 (39.0\%)   &$4.86$      \\
006 Flare 5&	$2.02_{\rm -0.79}^{+1.01}$	&	$1.51_{\rm -0.53}^{+0.58}$	  &436.0 (54.6\%)   &$2.75$      \\
007--008  &	$1.75_{\rm -0.83}^{+1.03}$	&	$1.94_{\rm -0.60}^{+0.64}$	  &518.3 (66.0\%)   &$2.22\times10^{-1}$      \\
009--012  &	$1.04_{\rm -0.36}^{+0.47}$	&	$1.48_{\rm -0.35}^{+0.39}$	  &576.9 (53.6\%)   &$8.82\times10^{-2}$      \\
007--012  &	$1.86_{\rm -0.44}^{+0.68}$	&	$1.92_{\rm -0.38}^{+0.43}$	  &1.09 (18)	    &$1.40\times10^{-1}$      \\
007--018  &	$2.04_{\rm -0.50}^{+0.62}$	&       $2.08_{\rm -0.37}^{+0.41}$	  &1.19 (19)	    &$5.96\times10^{-2}$	\\
  \hline
  \end{tabular}}
\smallskip
  $^{{a}}$ Last three digits of observation numbers, see Table~\ref{igr112:tab:alldata}, Col.~1. \\
  $^{{b}}$ Luminosity in the 1--10~keV band in units of $10^{35}$ erg s$^{-1}$ obtained from the spectral fits. \\
  $^{{c}}$ Cash statistics (C-stat) and percentage of Monte Carlo realizations that had statistic $<$C-stat.  		We performed $10^4$ simulations.
   \end{table}