\begin{table}%t6
\caption{\label{tab5}SN host spectral classification.}
%\centerline
{\begin{tabular}{ccccccc}%
\hline
\hline
SN &  T3850$^\dagger$ & Other  &  Comments & Host Spectral & Confidence 
 & ${\cal SN}$-fit  \\ 
 &  & indicators$^\ast$ &  & type$^\ddagger$& index $n_{\rm c}^\star$ &  \\
\hline
\object{1999cj}   & -- & [O~{\sc ii}], s. Mgb                            & red, likely E/S0 & 0      & 0.5 & Bulge   \\
\object{1999ck}   & -- & s. [O~{\sc ii}], w. H$\beta$, w. [O~{\sc iii}]         & poor gal. signal & 1      & 0.5 & Sa      \\
\object{1999dr}   & n. & s. H, K; B4000; s. Mgb                &  no emission       & 1      & 0.5 & Own gal.      \\
\object{1999dt}   & n. & s. [O~{\sc ii}]; s. H, K; B4000; s. H$\gamma$  & Sa/Sb            & 1      & 1   & Sb      \\
\object{1999du}   & -- & s. [O~{\sc ii}], H$\beta$, [O~{\sc iii}]               & clear ident. Sc  & 2      & 1   & Stb     \\
\object{1999dv}   &-- & s. H$\beta$, [O~{\sc iii}]                     & poor gal. signal   & 2      & 0.5 & Stb      \\
\object{1999dw}   & -- & w. [O~{\sc ii}]                                & poor S/N          & 1      & 0   & Sa      \\
\object{1999dx}   & y.& s. H, K; B4000; w. [O~{\sc ii}]; w H$\gamma$    & clear ident. E/S0& 0      & 1   & S0      \\
\object{1999dy}   & -- & [O~{\sc ii}]; [O~{\sc iii}]                            & faint            & 2      & 0.5 & Sb      \\
\object{1999dz}   & n. &  w. [O~{\sc ii}]; H, K                         & likely Sa/Sb     & 1      & 0.5 & Sb      \\
\object{1999ea}   & n. & s. [O~{\sc ii}]; [O~{\sc iii}]; H$\beta$; H, K       & Sa/Sb             & 1      & 1   & Sa      \\
\object{1999gx}   & --  & [O~{\sc ii}]; H, K                             & Sa/Sb            & 1      & 0.5 & Sa      \\
\hline
\end{tabular}}
\par
\smallskip
\hspace*{12mm}\footnotesize{Notes:}\\
\hspace*{15mm}\footnotesize{$^\dagger$ T3850~=~3850~\AA $\ $ CN trough present: y.~=~yes, 
n.~=~no; - = not identified}.\\
\hspace*{15mm}\footnotesize{$^\ddagger$ Type 0: spheroidal (E/S0); Type 1: early-type spiral (Sa/Sb); Type 2: late-type spiral (Sc/Starburst)}.\\
\hspace*{15mm}\footnotesize{$^\ast$ B4000~=~4000~\AA $\ $ break, s.~=~strong, w.~=~weak.}\\
\hspace*{15mm}\footnotesize{$^\star$ High confidence: $n_{\rm c}=1$; Average confidence: $n_{\rm c}=0.5$; Low confidence: $n_{\rm c}=0$.}
\end{table}