All Tables

Table 1: Coordinates and average Milky Way extinction (from Schlegel et al. 1998) of fields observed by the Deep/SN component of the CFHTLS.
Table 2: Average number of images and nights per band for each SNLS light-curve. Note that there is less data in $g_{\rm M}$ and $z_{\rm M}$ . The $\chi ^2_n$ column refers to the last fit that imposes equal fluxes on a given night. The expected value is 1.25 (due to pixel correlations), so we face a moderate scatter excess of about 12% over photon statistics. The larger values in $i_{\rm M}$ and $z_{\rm M}$ indicate that fringes play a role in this excess. The last column displays the average wavelength of the effective filters in Å.
Table 3: Cosmological parameters and statistical errors of Hubble diagram fits, with the BAO prior where applicable.
Table 4: Statistics of the 3 samples displayed in Fig. 11.
Table 5: Influence of a photometric calibration error on the cosmological parameters.
Table 6: Summary of uncertainties in the derived cosmological parameters. The dominant systematic uncertainty arises from the photometric calibration, itself dominated by the $i_{\rm M}$ and $z_{\rm M}$ band contributions.
Table 7: Transients from the first year sample identified as SNIa or SNIa*.
Table 8: Nearby type Ia supernovae.
Table 9: SNLS type Ia supernovae.