Table 6: List of the high redshift type Ia SNe used in this work. Columns are: IAU name, redshift, number of data points used in the fit, magnitude of the peak resulted from the fit (both statistical and systematic uncertainties are given) before Milky Way extinction correction, best fit template, $\chi ^2$ of the fit, Milky Way extinction in the J-band.
SN z s_B n $I_{\rm max}$ Template $\chi ^2$ $A_J^{{\rm MW}}$

SN 2000fr 0.543 1.034 $\pm$ 0.011 3 23.48 $\pm$ 0.08 $\pm$ 0.04 SN 1992bc 1.04 0.027

SN 1999ff 0.455 0.80 $\pm$ 0.05 2 23.55 $\pm$ 0.10 $\pm$ 0.08 SN 1996bl 0.05 0.022

**Table 6:** List of the high redshift type Ia SNe used in this work. Columns are: IAU name, redshift, number of data points used in the fit, magnitude of the peak resulted from the fit (both statistical and systematic uncertainties are given) before Milky Way extinction correction, best fit template, $\chi ^2$ of the fit, Milky Way extinction in the J-band.
SN	z	s_B	n	$I_{\rm max}$	Template	$\chi ^2$	$A_J^{{\rm MW}}$
SN 2000fr	0.543	1.034 $\pm$ 0.011	3	23.48 $\pm$ 0.08 $\pm$ 0.04	SN 1992bc	1.04	0.027
SN 1999ff	0.455	0.80 $\pm$ 0.05	2	23.55 $\pm$ 0.10 $\pm$ 0.08	SN 1996bl	0.05	0.022

Source LaTeX | All tables | In the text

	1 Introduction
	2 I-band light curve fitting
	3 The I-band Hubble diagram
	4 High redshift supernovae
	5 The I-band Hubble diagram up to $z \sim 0.5$
	6 SN Ia colours and intergalactic dust
	7 Test for SN brightness evolution
	8 Summary and conclusions
	References
	Online Material