\begin{table}%t3
 %\centering
\par
% \begin{minipage}{140mm}
  \caption{ Fits to the spectra of NGC~300 X-1 from Obs. 1--4,  and of IC~10 X-1. The first model is an absorbed power law plus Gaussian emission line, as favoured by Carpano et al. (2007a). For this model, we give absorption, normalised to 10$^{22}$ H atom~cm$^{-2}$, spectral index, line energy and width (in keV), and $\chi^2$/d.o.f.,  with good fit probability in square brackets. We only apply the Gaussian to NGC~300 X-1. We also give the 0.3--10~keV luminosity normalised to 10$^{37}$~erg  s$^{-1}$.  We next provide the best fits for a disk blackbody + power law model that is often used when describing the high state of disc-accreting BH XBs. We give the absorption, temperature of the disk blackbody, spectral index of the power law component and $\chi^2$. We then give 0.3--10~keV luminosity as before, and the fractional contribution of the power law model. }\label{specfits}
  \begin{tabular}{ccccccc}
  \hline\hline
  \noalign{\smallskip}
        &           &           &    NGC~300 X-1 &  & & IC~10 X-1  \\
  Model &  Parameter  & Obs. 1  &  Obs. 2 & Obs. 3 & Obs. 4 &  \\
\noalign{\smallskip}
 \hline
\noalign{\smallskip}  
PL + Line & $n_{\rm H}$ & 0.036  & 0.067(12)& 0.052(9) & 0.07(2) & 0.75(3)\\
 & $\Gamma$ &  2.46(6) & 2.44(7) & 2.44 & 2.53(8) & 2.56(6) \\
 & $E_{\rm Line}$ & 0.95 &  0.93(2) & 0.95(2) & 0.95(2) & $\dots$\\
 & $\sigma$ & 0.07 &  0.08(2)  & 0.07 & 0.06(3)  & $\dots$ \\
 & $\chi^2$/d.o.f. & 100/60 [9E--4] & 149/154 [0.60] & 50/60 [0.82]& 117/145 [0.05] & 794/652 [1E--4]\\
 & $L_{\rm 0.3-10~ keV}$ & 11.5(13) & 28.4(12) & 20(2) & 34.8(16) & 39(3)\\
\par
BB+PL & $n_{\rm H}$ & 0.11(4) & 0.130(12) & 0.22(5) & 0.17(3)& 0.92(10)\\
 & $kT$ & 1.02(14) & 1.02(17) & 0.92(12) & 1.08(15) & 0.82(3) \\
 & $\Gamma$ & 3.41(6) & 3.01(16) & 3.8(3) & 3.26(6) & 3.9(5)\\
 & $\chi^2$/d.o.f. & 52/58 [0.67] & 211/155 [2E--3] & 59/58[0.43] & 221/148[1.0E--4] & 697/650 [0.09]\\
&$L_{\rm 0.3-10 ~keV}$ & 16.9(17) & 39(2) & 49(6) & 59(3) & 91(19)\\
&Frac. PL & 0.80(11) & 0.93(14) & 0.91(18) & 0.92(6) & 0.93(3)\\
\par
DISKBB+PL & $n_{\rm H}$ & 0.12(4) & 0.13(4) & 0.22(9) & 0.17(4) & 0.84(4)\\
 & $kT_{\rm in}$ & 1.8(4) & 1.9(6) & 1.5(4) & 2.0(4) & 1.19(6)\\
 & $\Gamma$ & 3.6(7) & 3.1(4) & 4.1(7) & 3.4(3) & 3.9 \\
 & $\chi^2$/d.o.f. & 56/58 [0.54] & 213/155 [1.3E--3] & 62/58[0.33] & 226/148[3.0E--5] & 710/651 [0.05]\\
&$L_{\rm 0.3-10~ keV}$ & 19(3) & 33(25) & 49(6) & 53(5) & 72(9)\\
&Frac. PL & 0.89(17) & 0.6(7) & 0.91(18) & 0.93(11) & 0.86(19)\\
\hline
\end{tabular}
%\end{minipage}
\end{table}