\begin{table}%t2 \caption{\label{tab:tab1}Results of identifications of the SNLS 3rd year ESO-VLT SN~Ia and SN~Ia$\star$ spectra.} \small%\centering \par \begin{tabular}{llccclcc} \hline\hline SN name & Type & $z$ & $z$ source & $\Phi$ & Host model$^a$ & Host fraction & $\langle S/N\rangle^b$\\ \hline 03D1ar & Ia$\star$ &$0.408 \pm0.001$ & H & 5.3 & E(7) & 0.16 & 2.3 \\ 03D1bf & Ia$\star$ &$0.703 \pm0.001$ & H & --2.7 & E(3) & 0.16 & 1.4 \\ 03D1bm & Ia$\star$ &$0.575 \pm0.001$ & H & --5.1 & E(3) & 0.07 & 2.1 \\ 03D1bp & Ia$\star$ &$0.347 \pm0.001$ & H & --7.5 & E(2) & 0.86 & 2.2 \\ 03D1co & Ia &$0.679 \pm0.001$ & H & --4.1 & E(8) & 0.10 & 2.0 \\ 03D1dt & Ia &$0.612 \pm0.001$ & H & 5.1 & Sc(4) & 0.65 & 3.3 \\ 03D1fc & Ia &$0.332 \pm0.001$ & H & --4.4 & E(3) & 0.33 & 21.7 \\ 03D1fl & Ia &$0.687 \pm0.001$ & H & 0.5 & NoGalaxy & -- & 3.0 \\ 03D1gt & Ia &$0.560 \pm0.001$ & H & 7.0 & E(4) & 0.50 & 2.4 \\ 03D4ag & Ia$_{\rm pec}$ & $0.285\pm0.001$ & H & --8.6 & E(2) & 0.27 & 29.5 \\ 03D4at & Ia & $0.634\pm0.001$ & H & 5.5 & Sb-Sc & 0.42 & 3.7 \\ 03D4au & Ia$\star$ & $0.468\pm0.001$ & H & 6.5 & Sb-Sc & 0.43 & 5.2 \\ 03D4cx & Ia &$0.949 \pm0.014$ & S & 1.2 & NoGalaxy & -- & 0.6 \\ 03D4cx & Ia &$0.949 \pm0.014$ & S & 2.7 & S0(4) & 0.95 & 1.5 \\ 03D4cy & Ia &$0.927 \pm0.001$ & H & 4.6 & Sb-Sc & 0.16 & 0.5 \\ 03D4di & Ia$\star$ & $0.899 \pm0.001$ & H & --8.6 & Sb-Sc & 0.11 & 1.8 \\ 03D4di & Ia$\star$ & $0.899 \pm0.001$ & H & --6.5 & NoGalaxy & -- & 1.8 \\ 03D4dy & Ia & $0.61\pm0.01$ & S & 4.8 & NoGalaxy & -- & 5.5 \\ 03D4gf & Ia$\star$ &$0.580 \pm0.001$ & H & 20.4 & S0(1) & 0.46 & 1.5 \\ 03D4gg & Ia$\star$ &$0.592 \pm0.001$ & H & 16.4 & Sc(10) & 0.73 & 1.7 \\ 04D1ag & Ia & $0.557\pm0.001$ & H & 4.3 & E(12) & 0.08 & 5.4 \\ 04D1aj & Ia$\star$ &$0.721 \pm0.011$ & S & 11.6 & NoGalaxy & -- & 1.0 \\ 04D1aj & Ia$\star$ &$0.721 \pm0.011$ & S & 13.4 & NoGalaxy & -- & 1.2 \\ 04D1ak & Ia$\star$ &$0.526 \pm0.001$ & H & 11.8 & NoGalaxy & -- & 0.6 \\ 04D1dc & Ia & $0.211\pm0.001$ & H & --0.4 & NoGalaxy & -- & 33.4 \\ 04D1ff & Ia & $0.86\pm0.01$ & S & 4.6 & Sc(2) & 0.24 & 2.0 \\ 04D1hx & Ia &$0.560 \pm0.001$ & H & 5.9 & NoGalaxy & -- & 1.9 \\ 04D1iv & Ia &$0.998 \pm0.001$ & H & 3.0 & NoGalaxy & -- & 1.3 \\ 04D1jd & Ia$\star$ & $0.778\pm0.001$ & H & 6.8 & E(2) & 0.58 & 1.9 \\ 04D1kj & Ia &$0.585 \pm0.001$ & H & --3.7 & NoGalaxy & -- & 6.7 \\ 04D1ks & Ia &$0.798 \pm0.012$ & S & --1.0 & NoGalaxy & -- & 2.8 \\ 04D1ow & Ia &$0.915 \pm0.001$& H & 6.4 & NoGalaxy & -- & 1.6 \\ 04D1pc & Ia &$0.770 \pm0.001$ & H & 0.1 & E(3) & 0.22 & 3.0 \\ 04D1pd & Ia &$ 0.95\pm0.01$ & S & 2.5 & E(1) & 0.31 & 2.1 \\ 04D1pg & Ia &$0.515 \pm0.001$ & H & --1.3 & Sa-Sb & 0.61 & 8.9 \\ 04D1pp & Ia &$0.735 \pm0.001$ & H & 2.2 & NoGalaxy & -- & 1.2 \\ 04D1qd & Ia$\star$ & $0.767\pm0.001$ & H & --0.2 & E(1) & 0.71 & 4.8 \\ 04D1rh & Ia & $0.436\pm0.001$ & H & 0.0 & NoGalaxy & -- & 7.8 \\ 04D1rx & Ia$\star$ & 0.985$\pm0.001$ & H & 0.9 & NoGalaxy & -- & 1.4 \\ 04D1sa & Ia &$0.585 \pm0.001$ & H & --2.6 & E(1) & 0.72 & 6.4 \\ 04D1si & Ia &$0.702 \pm0.001$ & H & --1.7 & Sa(9) & 0.79 & 7.6 \\ 04D2ac & Ia &$0.348 \pm0.001$ & H & 1.3 & Sa-Sb & 0.20 & 7.6 \\ 04D2al & Ia &$0.836 \pm0.001$ & H & --2.5 & E(2) & 0.29 & 2.5 \\ 04D2an & Ia &$0.62 \pm 0.01$ & S & --3.4 & NoGalaxy & -- & 7.7 \\ 04D2an & Ia &$0.62 \pm 0.01$ & S & 0.3 & Sc(9) & 0.06 & 7.4 \\ 04D2bt & Ia & $0.220\pm0.001$ & H & 6.6 & E(6) & 0.01 & 9.2 \\ 04D2ca & Ia$\star$ &$0.835 \pm0.001$ & H & 12.0 & NoGalaxy & -- & 0.5 \\ 04D2ca & Ia$\star$ &$0.835 \pm0.001$ & H & 13.1 & NoGalaxy & -- & 0.9 \\ 04D2cc & Ia$\star$ &$0.838 \pm0.001$ & H & 6.1 & S0(3) & 0.66 & 1.8 \\ 04D2cc & Ia$\star$ &$0.838 \pm0.001$ & H & 7.2 & S0(2) & 0.67 & 1.5 \\ 04D2cf & Ia & $0.369\pm0.001$ & H & 8.5 & NoGalaxy & -- & 12.1 \\ 04D2cw & Ia$\star$ & $0.568\pm0.001$ & H & 19.3 & Sb-Sc & 0.58 & 1.4 \\ 04D2fp & Ia &$0.415 \pm0.001$ & H & 1.8 & NoGalaxy & -- & 11.5 \\ 04D2fs & Ia &$0.357 \pm0.001$ & H & 1.7 & NoGalaxy & -- & 17.8 \\ 04D2gc & Ia &$0.521 \pm0.001$ & H & --4.9 & E(1) & 0.19 & 5.2 \\ 04D2gp & Ia &$0.732 \pm0.001$ & H & 2.7 & NoGalaxy & -- & 2.5 \\ 04D2iu & Ia$\star$ &$ 0.70 \pm0.01$ & S & 9.8 & NoGalaxy & -- & 0.7 \\ 04D2iu & Ia$\star$ &$ 0.70 \pm0.01$ & S & 10.4 & E(1) & 0.09 & 1.2 \\ 04D2ja & Ia$\star$ &$0.740 \pm0.001$ & H & 9.2 & E(3) & 0.44 & 0.8 \\ 04D2ja & Ia$\star$ &$0.740 \pm0.001$ & H & 9.8 & E(3) & 0.19 & 0.5 \\ 04D2mc & Ia &$0.348 \pm0.001$ & H & 6.5 & Sa-Sb & 0.30 & 10.3 \\ 04D4an & Ia &$0.613 \pm0.001$ & H & 8.1 & NoGalaxy & -- & 0.8 \\ 04D4bk & Ia$\star$ & $0.88\pm0.01$ & S & 3.1 & E(1) & 0.20 & 1.6 \\ 04D4bq & Ia &$0.55 \pm0.01$ & S & 2.6 & NoGalaxy & -- & 2.6 \\ 04D4bq & Ia &$0.55 \pm0.01$ & S & 5.1 & NoGalaxy & -- & 6.5 \\ 04D4dw & Ia$\star$ & $1.031\pm0.001$ & H & 2.1 & Sa-Sb & 0.68 & 1.5 \\ \hline 04D4fx & Ia & $0.629\pm0.001$ & H & --8.4 & NoGalaxy & -- & 5.8 \\ 04D4gz & Ia$\star$ &$0.375 \pm0.001$ & H & --5.8 & Sa-Sb & 0.33 & 2.2 \\ 04D4gz & Ia$\star$ &$0.375 \pm0.001$ & H & 10.2 & NoGalaxy & -- & 1.8 \\ 04D4hf & Ia$\star$ &$0.936 \pm0.014$ & S & --0.5 & NoGalaxy & -- & 0.8 \\ 04D4ht & Ia &$0.217 \pm0.001$ & H & 6.6 & Sa-Sb & 0.62 & 3.9 \\ 04D4ib & Ia &$0.699 \pm0.001$ & H & 0.7 & S0-Sa & 0.71 & 4.2 \\ 04D4id & Ia &$0.769 \pm0.001$ & H & 3.0 & NoGalaxy & -- & 2.3 \\ 04D4ht & Ia &$0.217 \pm0.001$ & H & 6.6 & Sa-Sb & 0.62 & 3.9 \\ 04D4ib & Ia &$0.699 \pm0.001$ & H & 0.7 & S0-Sa & 0.71 & 4.2 \\ 04D4id & Ia &$0.769 \pm0.001$ & H & 3.0 & NoGalaxy & -- & 2.3 \\ 04D4jr & Ia & $0.47\pm0.01$ & S & --5.9 & NoGalaxy & -- & 16.5 \\ 04D4ju & Ia & $0.472\pm0.001$ & H & --2.2 & S0(1) & 0.44 & 3.5 \\ 04D4jw & Ia$\star$ & 0.961$\pm0.001$ & H & 2.2 & S0-Sa & 0.69 & 2.3 \\ 05D1cb & Ia &$0.632 \pm0.001$ & H & 4.3 & Sb-Sc & 0.28 & 4.5 \\ 05D1ck & Ia &$0.617 \pm0.001$ & H & --2.7 & Sb-Sc & 0.39 & 0.7 \\ 05D1cl & Ia$\star$ & $0.83\pm0.01$ & S & 8.7 & Sd(4) & 0.36 & 1.8 \\ 05D1dn & Ia & $0.566\pm0.001$ & H & --4.7 & NoGalaxy & -- & 7.3 \\ 05D1hk & Ia$_{\rm pec}$ & 0.263$\pm0.001$ & H & --5.0 & Sc(5) & 0.39 & 21.4 \\ 05D1hn & Ia & $0.149\pm0.001$ & H & --1.0 & NoGalaxy & -- & 13.0 \\ 05D1iz & Ia$\star$ & $0.86\pm0.01$ & S & 7.8 & Sd(1) & 0.24 & 2.1 \\ 05D1ke & Ia & $0.69\pm0.01$ & S & 2.2 & NoGalaxy & -- & 4.9 \\ 05D2ac & Ia & $0.479\pm0.001$ & H & 2.0 & NoGalaxy & -- & 10.9 \\ 05D2ay & Ia$\star$ & $0.92\pm0.01$ & S & 5.8 & S0(1) & 0.07 & 1.1 \\ 05D2bt & Ia & $0.68\pm0.01$ & S & 1.4 & NoGalaxy & -- & 2.1 \\ 05D2bv & Ia & $0.474\pm0.001$ & H & --0.1 & Sb-Sc & 0.26 & 8.3 \\ 05D2bw & Ia & $0.92\pm0.01$ & S & 1.9 & Sb-Sc & 0.25 & 2.1 \\ 05D2by & Ia$\star$ &$0.891 \pm0.001$ & H & 0.9 & Sc(11) & 0.83 & 1.3 \\ 05D2cb & Ia$\star$ &$0.427 \pm0.001$ & H & --5.8 & Sc(11) & 0.57 & 2.9 \\ 05D2ci & Ia &$0.630 \pm0.001$ & H & 3.6 & NoGalaxy & -- & 0.8 \\ 05D2ci & Ia &$0.630 \pm0.001$ & H & 4.9 & NoGalaxy & -- & 0.7 \\ 05D2ci & Ia &$0.630 \pm0.001$ & H & 6.7 & NoGalaxy & -- & 1.4 \\ %05D2cl & Ia$\star$ & 0.857$\pm0.001$ & H & 6.8 & E(2) & 0.86 & 1.8 \\ 05D2ct & Ia$\star$ &$0.734 \pm0.001$ & H & 7.8 & Sd(11) & 0.63 & 4.6 \\ 05D2dt & Ia &$0.574 \pm0.001$ & H & --1.7 & E(3) & 0.43 & 6.0 \\ 05D2dw & Ia &$0.417 \pm0.001$ & H & --5.3 & S0(1) & 0.12 & 10.3 \\ 05D2dy & Ia &$0.51 \pm 0.01$ & S & 1.1 & Sb-Sc & 0.02 & 4.8 \\ 05D2eb & Ia &$0.534 \pm0.001$ & H & --4.7 & S0(1) & 0.04 & 6.2 \\ 05D2ec & Ia &$0.640 \pm0.001$ & H & 2.7 & NoGalaxy & -- & 2.4 \\ 05D2ei & Ia$\star$ &$0.366 \pm0.001$ & H & 16.9 & S0(4) & 0.55 & 2.5 \\ 05D2fq & Ia &$0.733 \pm0.001$ & H & 2.1 & NoGalaxy & -- & 1.9 \\ 05D2he & Ia &$0.608 \pm0.001$ & H & 3.0 & E(1) & 0.26 & 3.1 \\ 05D2ie & Ia &$ 0.348\pm0.001$ & H & --8.9 & Sc(4) & 0.45 & 4.4 \\ 05D2nn & Ia & $0.87\pm0.01$ & S & --1.3 & Sa(8) & 0.26 & 1.9 \\ 05D4af & Ia & $0.499\pm0.001$ & H & 11.3 & NoGalaxy & -- & 8.8 \\ 05D4ag & Ia$\star$ & $0.64\pm0.01$ & S & 14.0 & Sb-Sc & 0.10 & 2.0 \\ 05D4ay & Ia$\star$ & $0.408\pm0.001$ & H & 8.2 & Sa-Sb & 0.80 & 2.55 \\ 05D4ay & Ia$\star$ & $0.408\pm0.001$ & H & 9.6 & Sa-Sb & 0.80 & 1.8 \\ 05D4be & Ia &$0.537 \pm0.001$ & H & 3.9 & E(1) & 0.31 & 5.5 \\ 05D4bi & Ia &$0.775 \pm0.001$ & H & --1.5 & Sc(1) & 0.40 & 3.7 \\ 05D4bj & Ia &$0.701 \pm0.001$ & H & --2.0 & Sc(9) & 0.68 & 2.8 \\ 05D4cn & Ia &$0.763 \pm0.001$ & H & 4.7 & S0(1) & 0.27 & 3.0 \\ 05D4cq & Ia &$0.701 \pm0.001$ & H & --0.1 & NoGalaxy & -- & 4.6 \\ 05D4cs & Ia &$ 0.79 \pm0.01$ & S & --1.7 & Sc(12) & 0.16 & 4.3 \\ 05D4cw & Ia &$0.375 \pm0.001$ & H & 7.0 & S0(6) & 0.57 & 16.4 \\ 05D4dw & Ia &$0.855 \pm0.001$ & H & 4.7 & Sc(12) & 0.19 & 0.9 \\ 05D4ef & Ia$\star$ & $0.605\pm0.001$ & H & 3.5 & E(3) & 0.78 & 1.6 \\ 05D4ej & Ia &$0.585 \pm0.001$ & H & 7.6 & NoGalaxy & -- & 3.5 \\ 05D4ek & Ia &$0.536 \pm0.001$ & H & 2.1 & NoGalaxy & -- & 8.2 \\05D4ev & Ia & $0.722\pm0.001$ & H & --3.6 & NoGalaxy & -- & 3.4 \\ 05D4fe & Ia$\star$ &$0.984 \pm0.001$ & H & --2.0 & E(3) & 0.65 & 1.1 \\ 05D4ff & Ia$\star$ &$0.402 \pm0.001$ & H & 5.1 & Sc(6) & 0.83 & 4.9 \\ 05D4fg & Ia &$0.839 \pm0.001$ & H & --0.3 & S0(5) & 0.32 & 2.3 \\ 06D1ab & Ia &$0.182 \pm0.001$ & H & --4.4 & E(7) & 0.11 & 13.9 \\ 06D2bk & Ia &$0.499 \pm0.001$ & H & 0.9 & Sb-Sc & 0.15 & 3.8 \\ 06D2ca & Ia &$0.531 \pm0.001$ & H & 0.0 & Sd(5) & 0.27 & 3.2 \\ 06D2ca & Ia &$0.531 \pm0.001$ & H & 0.7 & Sd(3) & 0.18 & 2.5 \\ \hline 06D2cb & Ia$\star$ & $1.00\pm0.01$ & S & 3.0 & NoGalaxy & -- & 1.7 \\ 06D2cc & Ia & $0.532\pm0.001$ & H & 3.3 & NoGalaxy & -- & 6.2 \\ %new 06D2cd & Ia & $0.930\pm0.001$ & H & 4.2 & NoGalaxy & -- & 5.8 \\ %new 06D2ce & Ia & $0.82\pm0.01$ & S & 0.0 & NoGalaxy & -- & 7.3 \\ 06D2ck & Ia$\star$ & $0.552\pm0.001$ & H & 7.7 & Sa-Sb & 0.24 & 1.6 \\ 06D2ga & Ia$\star$ & $0.84\pm 0.01$ & S & 5.4 & Sb-Sc & 0.19 & 2.0 \\ 06D4ce & Ia &$0.85 \pm0.01$ & S & 2.7 & NoGalaxy & -- & 2.3 \\ 06D4ce & Ia &$0.85 \pm0.01$ & S & 3.3 & NoGalaxy & -- & 2.7 \\ 06D4cl & Ia &$1.00 \pm 0.01$ & S & --2.5 & E(1) & 0.01 & 2.5 \\ 06D4co & Ia &$0.437 \pm0.001$ & H & 3.5 & E-S0 & 0.58 & 12.8 \\ 06D4cq & Ia &$0.411 \pm0.001$ & H & --1.4 & NoGalaxy & -- & 8.2 \\ \hline \end{tabular} \smallskip $^a$ Host type of the best fitting model. The number in parenthesis is the age of the best fitting PEGASE template (in Gyrs). Two host types separated by a dash indicate that the best fitting host model is an interpolation between two \citet{Kinney96} templates. The label ``NoGalaxy'' denotes that the best fitting model is obtained with no host model.\\ $^b$ Average signal-to-noise ratio per 5~\AA\ pixel. \end{table}