\begin{table}%t7
\caption{\label{tab:gemprop} SNLS identifications and derived properties for SNe candidates observed from Nov.~2004 to May 2006.} 
%\centerline
 {\begin{tabular}{llllll}
\hline \hline
\noalign{\smallskip}
SN     & $z$   & $\sigma_{z}^{ {a}} $ & CI \& Type$^{ {b}}$  & Template$^{ {c}}$ & $z$ from$^{ {d}}$ \\
\hline
04D1pu & 0.639 & 0.001 & 3 - SN Ia*& ...      & OII \\
04D2mh & 0.59  & 0.01  & 3 - SN Ia*& 1996X +2  & SN \\
04D2mj & 0.513 & 0.001 & 5 - SN Ia & 1992A --1  & OII, H$\beta$, OIII \\
05D1az & 0.842 & 0.001 & 5 - SN Ia & 1996X +2  & possible OII  \\
05D1by & 0.298 & 0.001 & 5 - SN Ia & 2002bo --1 & H$\alpha$, H$\beta$, OIII, SII \\
05D1bz & ...   & ...   & 2 - SN   & ...      & ... \\
05D1cc & 0.564 & 0.001 & 5 - SN Ia & 1996X +7  & H$\beta$, OII, OIII \\
05D1ee & 0.558 & 0.001 & 4 - SN Ia & 1992A +6  & H\&K \\
05D1ej & 0.312 & 0.001 & 4 - SN Ia & 1989B --5  & NII \\
05D1em & 0.866 & 0.001 & 5 - SN Ia & 1999ee +5 & nearby galaxy\\
05D1eo & 0.737 & 0.001 & 2 - SN & ...      & H\&K, OII \\
05D1er & 0.85  & 0.01  & 3 - SN Ia*& 1999aa --1& SN \\
05D1hn & 0.149 & 0.001 & 5 - SN Ia & 2003du --7 & H$\alpha$, SII, OII \\
05D1ju & 0.707 & 0.001 & 3 - SN Ia*& 1996X +7 & OII, OIII \\
05D1ka & 0.857 & 0.001 & 2 - SN & ...      & H\&K \\
05D1kl & 0.560 & 0.001 & 3 - SN Ia*& 1990N --7 & OII, OII \\
05D2ab & 0.323 & 0.001 & 5 - SN Ia & 1998bu --4 & H$\alpha$ \\
05D2ah & 0.184 & 0.001 & 5 - SN Ia & 1994D --5  & H$\alpha$, SII \\
05D2ck & 0.698 & 0.001 & 5 - SN Ia & 1992A +6  & H\&K \\
05D2ja & 0.303 & 0.001 & 5 - SN Ia & 1999aw +16 & H$\alpha$, SII, OIII \\
05D2nt & 0.757 & 0.001 & 4 - SN Ia & 1999ee +3 & OII,H$\beta$, OIII \\
05D2ob & 0.924 & 0.001 & 4 - SN Ia & 1989B --1 & OII \\
05D3ax & 0.643 & 0.001 & 5 - SN Ia & 1999aw +12& OII, OIII \\
05D3bt & 0.462 & 0.001 & 2 - SN  & ... &   H$\beta$, OII, OIII \\
05D3cf & 0.419 & 0.001 & 4 - SN Ia & 1999be +19& H$\beta$, OII, OIII \\
05D3ci & 0.515 & 0.001 & 5 - SN Ia & 1992A --5  & OII, H\&K \\
05D3cq & 0.890 & 0.001 & 3 - SN Ia*& 1999ao +5 & H$\beta$, OII \\
05D3cx & 0.805 & 0.001 & 4 - SN Ia & 1999bk +7 & possible OII \\
05D3jq & 0.579 & 0.001 & 4 - SN Ia & 2000E +5& H$\beta$, H$\gamma$, OII \\
05D3ki & 0.965 & 0.001 & 2 - SN & ...      &  OII \\
05D3km & 0.97  & 0.01 & 3 - SN Ia* & 1999bo +1& SN \\
05D3kp & ...   & ...  &  2 - SN    & ...      & ... \\
05D3kt & 0.648 & 0.001 & 5 - SN Ia & 1999ee --2 & H$\beta$, OII, OIII \\
05D3lb & 0.647 & 0.001 & 5 - SN Ia & 1999ee 0  & H$\beta$, OII, OIII \\
05D3lc & 0.461 & 0.001 & 3 - SN & ...       & H\&K \\
05D3lw & 0.601 & 0.001 & 2 - SN & ...      & OII \\
05D3mn & 0.760 & 0.001 & 3 - SN Ia*& 1999av +2   & possible OII \\
05D3mh & 0.67  & 0.01 &  4 - SN Ia & 1998aq --8 & SN \\
05D3mq & 0.246 & 0.001 & 5 - SN Ia & 1992A +9  & H$\alpha$ \\
05D3mx & 0.46  & 0.01 &  4 - SN Ia & 1998bu +8 & SN \\
05D3ne & 0.169 & 0.001 & 5 - SN Ia & 1994D --4  & SDSS host spectrum \\
05D4av & 0.509 & 0.001 & 3 - SN Ia*& 2002bo --4 & OII \\
05D4bm & 0.375 & 0.001 & 5 - SN Ia & 1996X --1  & H$\beta$, OII, OIII \\
05D4ca & 0.607 & 0.001 & 2 - SN & 1988A +3& H$\beta$, OII, OIII \\
05D4cn & 0.763 & 0.001 & 3 - SN Ia*& 2002bo --1& OII, H\&K \\
05D4dt & 0.407 & 0.001 & 4 - SN Ia & 1994D --2 & H$\alpha$,OII, H\&K, H$\beta$, OIII \\
05D4dx & 0.793 & 0.001 & 3 - SN Ia*& 1002A +5 & H\&K, H$\delta$ \\
05D4dy & 0.79  & 0.01  & 4 - SN Ia & 1994D +2 & SN \\
05D4fn & 0.4   & 0.1   & 2 - SN & ...      & SN \\
05D4fo & 0.373 & 0.001 & 5 - SN & 1994D --2 & H$\alpha$, H\&K \\
05D4gw & 0.808 & 0.001 & 5 - SN Ia & 1999bp --2 & OII \\
05D4hn & 0.842 & 0.001 & 4 - SN Ia & 1981B 0   & OII, OIII \\
06D3bz & 0.72  & 0.01  & 4 - SN Ia & 1989B --1 & SN \\
06D3cb & ...   & ...   & 2 - SN & ...      & ... \\
06D3cc & 0.90  & 0.01  & 3 - SN Ia*  & 1990N --7 & ... \\
06D3cl & 0.555 & 0.001 & 2 - SN & ...      & OII, OIII, H$\beta$ \\
06D3cn & 0.818 & 0.001 & 5 - SN Ia & 1996X --1 & OII, OIII, H$\beta$ \\
06D3du & 1.0   & 0.1   & 2 - SN & ...      & SN \\
06D3dz & 0.294 & 0.001 & 2 - SN & ... & H$\alpha$, SII \\
\hline
\end{tabular}}
\par
\smallskip
 {{ $^a$  Redshifts identified with host galaxy features are accurate to $\approx $$\pm$$ 0.001$; redshifts identified;}} \\ 
 {{ with template matches are accurate to $\approx $$\pm $$0.01$;}} \\
 {{ $^b$   Final object identification and confidence index;}} \\
 {{ $^c$   Best low-$z$ spectral fit (name and days past max.);}} \\
 {{ $^d$   The host features used to estimate $z$.}}  \\
\par
\end{table}