Table 3: List of SNe used in the Hubble diagram. is the peak magnitude corrected for dust extinction and for the width-luminosity relation, following Eq. (1). The quoted uncertainties do not include the redshift contribution due to peculiar velocities in the host galaxies, assumed equal to 300 km s^-1. Redshifts from Table 2 are here transformed into the CMB frame.

SN	sB
1992al	0.917 0.012	0.014	14.868 0.162
1992bc	1.076 0.008	0.020	15.718 0.111
1992bg	0.952 0.017	0.036	17.120 0.107
1992bh	1.014 0.022	0.045	17.637 0.062
1992bo	0.741 0.008	0.017	15.710 0.138
1992bp	0.863 0.022	0.079	18.689 0.055
1993H	0.773 0.011	0.025	16.169 0.106
1993O	0.887 0.012	0.053	17.967 0.054
1993ag	0.909 0.027	0.050	17.928 0.069
1994M	0.810 0.016	0.024	16.080 0.111
1994T	0.911 0.025	0.036	17.105 0.085
1995bd	1.172 0.026	0.014	14.939 0.162
1996C	1.039 0.013	0.027	16.669 0.097
1996bl	0.924 0.016	0.035	16.630 0.070
1996bo	0.890 0.011	0.016	14.860 0.138
1997bq	0.912 0.009	0.010	14.154 0.219
1997dg	0.836 0.057	0.030	16.740 0.110
1997E	0.784 0.008	0.013	14.888 0.173
1998ab	0.921 0.010	0.028	16.180 0.083
1998es	1.093 0.014	0.010	13.885 0.219
1998V	0.922 0.013	0.017	15.272 0.131
1999aa	1.073 0.005	0.015	15.250 0.146
1999ac	1.079 0.009	0.010	14.144 0.218
1999dq	1.037 0.000	0.014	14.382 0.155
1999gp	1.154 0.011	0.026	16.303 0.090
2000cn	0.749 0.000	0.023	16.114 0.107
2000dk	0.716 0.007	0.016	15.375 0.147
2000fa	1.019 0.010	0.022	16.029 0.106