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Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 85-103 Full HTML
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Table 2:

Results of identifications of the SNLS 3rd year ESO-VLT SN Ia and SN Ia$\star $ spectra.
SN name Type z z source $\Phi$ Host modela Host fraction $\langle S/N\rangle^b$
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
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
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
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
06D2cd Ia $0.930\pm0.001$ H 4.2 NoGalaxy - 5.8
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 $1.00\pm0.01$ 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

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 Kinney et al. (1996) templates. The label ``NoGalaxy'' denotes that the best fitting model is obtained with no host model.
b Average signal-to-noise ratio per 5 Å pixel.

Source LaTeX | All tables | In the text

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