Table 7: SNLS identifications and derived properties for SNe candidates observed from Nov. 2004 to May 2006.

SN		 z $\sigma_{z}^{ {a}} $ CI & Type b Template c z from d
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
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.


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