\begin{table}%t3
\caption {\label{spec1122}Spectral fit parameters for GRB~061122 with spectral models as described in Sect.~\ref{SA} and reduced $\chi^2$ per degrees of freedom (d.o.f.). }
%\centerline
 {
\begin{tabular}{clcccccc}
\hline\hline
  Detector &  Spectral  &  $\alpha$$^a$ &   $\beta$ &   $E_{0}$/kT  & $E_{\rm peak}$ &  $\chi^2_{\rm red}$ &   Fluence$^b$  \\
&  model & & &   (keV) &   (keV) &  /d.o.f. &   ($ 10^{-6}$ erg cm$^{-2}$) \\
\hline%\\[-3mm]
& PL & --1.67 & ... & ... & ... & 3.92/58 & $\rm 17.79 ^{+0.23}_{-0.32}$ \\[1mm]
SPI$^c$ & GRBM & $\rm -0.98^{+0.11}_{-0.12}$ & $\rm -2.72^{+0.34}_{-0.85}$ &
$166^{\rm +39}_{-28}$ & $\rm 169^{+44}_{-35}$& 1.19/56 & $\rm 19.63 ^{+0.16}_{-0.71}$ \\[1mm]
& BB+PL & $\rm -1.81^{+0.08}_{-0.07}$ & ...  & $36\pm 3$ & ... &1.21/56 & $19.96 ^{\rm +0.54}_{-0.71}$\\[1mm]
& Cutoff PL & $\rm -1.01^{+0.10}_{-0.11}$ & ... & ... & $\rm 179^{+38}_{-28}$ & 1.24/57 & $\rm 19.64^{+0.64}_{-1.47}$\\
%& & & & & & & \\
& PL & --1.47 & ... & ... & ... & 2.30/92 & $\rm 5.13 ^{+0.09}_{-0.11}$ \\[1mm]
Joint Fit & GRBM & $\rm -1.14^{+0.27}_{-0.32}$ & $\rm -1.91^{+0.07}_{-0.10}$  & $\rm 81^{+120}_{-70}$ & $\rm 70^{+106}_{-63}$ & 1.35/90 & $\rm 8.80 ^{+0.11}_{-4.62}$ \\[1mm]
(IBIS \& SPI) & BB+PL & $-1.74 \pm 0.07$ & ... & $\rm 15^{+4}_{-3}$ & ... & 1.40/90 & $\rm 8.36 ^{+0.04}_{-0.29}$ \\[1mm]
& Cutoff PL & $\rm -0.97^{+0.12}_{-0.13}$ & ... & ... & $\rm 129^{+45}_{-29}$ & 1.45/91 & $\rm 5.10^{+0.33}_{-0.60}$\\
%& & & & & & & \\
KONUS$^d$ & Cutoff PL & $\rm -1.03^{+0.06}_{-0.07}$ & ... & ... & $\rm 160^{+8}_{-7}$ & 1.03/62 & $\rm 23.1^{+0.5}_{-1.2} $ \\[1mm]
\hline
\end{tabular}}
\par
\smallskip
$^a$   {Low energy photon index in the Band model/single power-law index for the PL/BB+PL/Cutoff PL models.}
$^b$  {20--200~keV.}
\par
$^c$   {20~keV--8~MeV.}
$^d$ {KONUS-WIND spectral parameters are taken from \cite{gcn5841} and are in the energy range 20~keV--2~MeV.}
\par
\end{table}