Table 4: Results from ${\cal SN}$-fit using peculiar SN Ia templates.
SN Telescope Peculiar Normal F-test
    --------------------- --------------- probability (%)
    Best-fit Phase $\chi ^2$ d.o.f. Phase $\chi ^2$ d.o.f.  
1999cj WHT 99aa1 +14 1.025 859 +9 1.005 859 57
1999ck WHT 99aa -7 1.309 533 -9 1.171 502 1.9
1999dr WHT 00cx2 +30 1.100 900 +24 0.949 935 $2.2\times 10^{-3}$
1999dt WHT 99aa -7 1.523 667 -9 1.245 623 $6\times 10^{-4}$
1999du WHT 99aa -7 0.945 894 -9 0.867 853 1.7
1999dv WHT 99aa -7 1.443 833 -7 0.994 436 $2\times 10^{-20}$
1999dw WHT 99aa -7 0.764 643 -4 0.746 705 52
1999dx WHT 99aa -3 1.825 935 +5 1.654 935 0.4
1999dy WHT 99aa -3 2.508 932 0 1.136 934 <10-20
1999dz WHT 00cx -3 1.263 563 -4 1.169 971 0.8
1999ea WHT 99aa -11 1.321 804 -8 1.117 697 10-2
1999gx WHT 91T3 -12 0.939 674 -4 0.938 794 97
1999du NOT 00cx +14 0.883 336 +6 0.812 572 2.7
1999dv NOT 99aa +14 1.429 542 +9 1.153 637 $4\times 10^{-5}$
Notes:
1 Spectral template from Garavini et al. (2004).
2 Spectral template from Li et al (2001c).
3 Spectral template from Mazzali et. al. (1995).

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