\begin{table}%t2
\caption{\label{tab2} Results from ${\cal SN}$-fit.}
%\centerline
{\begin{tabular}{ccccccccc}
\hline \hline
SN     & Telescope & Best fit SN& \% (host)$^\dagger$ & $z_{\rm f}$  & $z_{\rm h}$  & Spectroscopic & Reduced & d.o.f.$^\ast$ \\
name & & template (reference) & & & & phase$^\ddagger$ & $\chi^2$ &\\ 
\hline
\object{1999cj} &   WHT   & 92A (Kirshner \etal 1993)& 31(Bulge)           & 0.355       & 0.362  & +9   & 1.00 & 859\\
\object{1999ck} &   WHT   & 94D (Patat \etal 1996) & 48(Sa)                & 0.434       & 0.432  & $-$9   & 1.17 & 502 \\
\object{1999dr}$^1$ &  WHT &94D (Patat \etal 1996) &  48(own galaxy)       & 0.174       & 0.178  & +24  & 0.95 & 935\\
\object{1999dt} & WHT &94D (Patat \etal 1996) &  80(Sb)                & 0.438       & 0.437  & $-$9   & 1.24 & 623 \\
\object{1999du}$^2$ &  WHT &99ee (Hamuy \etal 2002) &  65(Stb4)            & 0.258       & 0.260  & $-$9  & 0.87 & 853\\
\object{1999dv} &  WHT &03du (Anupama \etal 2005) &  11(Stb1)              & 0.177       & 0.186  & $-$7   & 0.99 & 936\\
\object{1999dw} &  WHT &99ee (Hamuy \etal 2002) &  63(Sa)                  & 0.464       & 0.460  & $-$4   & 0.75 & 705\\
\object{1999dx} &  WHT &92A (Kirshner \etal 1993) &  77(S0)                & 0.270       & 0.269  & +5   & 1.66 & 935 \\
\object{1999dy} &  WHT &96X (Salvo \etal 2001) &  23(Sb)                   & 0.202       & 0.215  &  0   & 1.14 & 934\\
\object{1999dz} &  WHT &99ee (Hamuy \etal 2002) &  79(Sb)                  & 0.480      & 0.486  & $-$4   & 1.17 & 671\\
\object{1999ea} &  WHT &94D (Patat \etal 1996) &  42(Sa)                   & 0.398       & 0.397  & $-$8   & 1.12 & 697\\
\object{1999gx}      & WHT & 94D (Patat \etal 1996) & 64(Sa)                    & 0.487       & 0.493 & $-$4 & 0.93 & 871\\
\object{1999du}$^1$ &  NOT &92A (Kirshner \etal 1993) & 28(own galaxy)         & 0.250       & 0.260 & +6 & 0.81 & 572\\
\object{1999dv}  &  NOT &92A (Kirshner \etal 1993) & 6(Sc)                 & 0.181 & 0.186 & +9 & 1.15 & 637\\
\hline
\end{tabular}}
\par
\smallskip
\footnotesize{Notes:}\\
\hspace*{5mm}\footnotesize{$^\dagger$ \%(host) = $\beta/(\alpha + \beta)\times 100$ (see text).}\\
\hspace*{5mm}\footnotesize{$^\ddagger$ Typical error is $\pm 3$ days.}\\
\hspace*{5mm}\footnotesize{$^\ast$ Number of degrees of freedom.}\\
\hspace*{5mm}\footnotesize{$^1$ The observed galaxy has been used
  for the fit.}\\
\hspace*{5mm}\footnotesize{$^2$ Best solution when emission lines are
  ignored: 99ee $-$9~days, 39\% (Sb), $z_{\rm f}=0.261$, reduced $\chi^2=0.78$, d.o.f.~=~936.}\\
\end{table}