\begin{table}%t5
\caption{\label{tabLCDMfull}Robustness of the full-sky fit to the
flat $\Lambda$CDM model at arbitrary redshift. The fit parameters
are the calibration $H_0/H_0^*$ and the dimensionless matter density
$\Omega_{\rm M}$. We compare the number of degrees of freedom (d.o.f.),
$\chi^2$/d.o.f., and the best fit cosmological parameters for data sets
A, B, and C for various assumptions on the acceptable light
extinction $A_{\rm V}$, peculiar velocity dispersion $\sigma_v$, intrinsic dispersion $\sigma_{\rm int}$
and redshift interval included in the fit.}
%\centering
\par
\begin{tabular}{lcccc}
 \hline\hline\noalign{\smallskip}
 & d.o.f. & $\frac{\chi^2}{\rm d.o.f.}$ & $\frac{H_0}{H_0^*}$ & $\Omega_{\rm M}$ \\\noalign{\smallskip}
\hline
{\bf data set A:} 253 SNe, $z \in [0.002,1.755]$\\
$A_{\rm V} \leq 1$, $\sigma_v = 345$ km~s$^{-1}$, $z$ arbitrary & 242 &1.31 & $  1.02\pm0.02 $&$  0.31\pm0.06 $ \\
$\sigma_v = 230$ km~s$^{-1}$ & 242 & 1.62 &$ 1.02 \pm 0.02$ & $ 0.31 \pm 0.06$ \\
$\sigma_v = 460$ km~s$^{-1}$ & 242 & 1.14 &$ 1.01 \pm 0.02$ & $ 0.34 \pm 0.06 $\\
$\sigma_v = 690$ km~s$^{-1}$ & 242 & 0.96 &$ 1.01 \pm 0.02$ & $ 0.34 \pm 0.07 $\\
%$\sigma_v = 1150$ km~s$^{-1}$ & 242 & 0.80 &$ 1.01 \pm 0.02$ & $ 0.34 \pm 0.08$ \\
$0.0 < z \leq 0.2$    & 137 & 1.27 &$ 1.03 \pm 0.03$ & $ 0.04^{ +0.66}_{ -0.04} $\\
$0.01<z$              & 211 & 1.20 &$ 1.01 \pm 0.02$ & $ 0.34 \pm 0.07 $\\
$A_{\rm V} \leq 0.5$        & 219 & 1.26 &$ 1.01 \pm 0.02$ & $ 0.32 \pm 0.07 $\\
\hline
{\bf data set B:} 186 SNe, $z\in [0.010, 1.755]$\\
$A_{\rm V} \leq 1$, $\sigma_v = 345$ km~s$^{-1}$, $z$ arbitrary & 180 & 1.11 & $ 0.98 \pm 0.02$&$ 0.32 \pm0.06 $ \\
$\sigma_v = 230$ km~s$^{-1}$ & 180 & 1.14 & $0.98\pm 0.02$ & $ 0.32\pm 0.06 $ \\
$\sigma_v = 460$ km~s$^{-1}$ & 180 & 1.07 & $ 0.98\pm 0.02$ &$ 0.32 \pm 0.06 $\\
$\sigma_v = 690$ km~s$^{-1}$ & 180 & 1.00 & $ 0.98\pm 0.02$& $0.32 \pm 0.06 $\\
%$\sigma_v = 1150$ km~s$^{-1}$ & 180 & 0.91 & $ 0.97\pm 0.03 $&$ 0.34 \pm 0.08$ \\
$0.0 < z \leq 0.2$      & \ 75 & 0.84 &$ 1.00\pm 0.02 $&$\leq$ 0.96 ($2\sigma$)\\
$A_{\rm V} \leq 0.5$           & 159 & 0.94 &$ 0.97 \pm 0.02 $&$ 0.32 \pm 0.06 $\\
\hline
{\bf data set C:} 117 SNe, $z\in [0.015, 1.01]$\\
$A_{\rm V} \leq 1$, $\sigma_v = 345$ km~s$^{-1}$, $\sigma_{\rm int}=0.03$, $z$ arbitrary & 115 & 1.02 & $ 1.08 \pm 0.03$&$ 0.25 \pm 0.07$ \\
$\sigma_v = 230$ km~s$^{-1}$ & 115 & 1.05 & $1.08\pm 0.05$ & $ 0.23\pm 0.07 $ \\
$\sigma_v = 460$ km~s$^{-1}$ & 115 & 0.99 & $ 1.08\pm 0.02$ &$ 0.23 \pm 0.06 $\\
$\sigma_v = 690$ km~s$^{-1}$ & 115 & 0.93 & $ 1.08\pm 0.03 $& $0.23 \pm 0.06 $\\
%$\sigma_v = 1150$ km~s$^{-1}$ & 115 & 0.85 & $ 1.07\pm 0.03 $&$ 0.26 \pm 0.08 $ \\
$0.0 < z \leq 0.2$      & \ 42 & 0.84 &$ 1.08 \pm 0.04 $&$ 0.20^{ +1.48}_{ -0.20} $\\
$\sigma_{\rm int}=0 $     & 115 & 8.60 & $ 1.08 \pm 0.01$&$ 0.27 \pm 0.03$ \\
$\sigma_{\rm int}=0.02  $ & 115 & 1.68 & $ 1.08 \pm 0.05$&$ 0.24 \pm 0.02$ \\
\hline
\end{tabular}
\end{table}