Table 8: Restframe B-I colours in magnitudes for the two high redshift SNe. The Epoch is in restframe days relative to the B-band maximum, divided by the B-band stretch.
Epoch B-I

SN 2000fr

-0.32 -0.51 $\pm$ 0.12

14.70 -0.50 $\pm$ 0.24

29.08 1.42 $\pm$ 0.17

SN 1999ff

5.59 -0.18 $\pm$ 0.13

27.20 1.38 $\pm$ 0.24

**Table 8:** Restframe B-I colours in magnitudes for the two high redshift SNe. The Epoch is in restframe days relative to the B-band maximum, divided by the B-band stretch.
Epoch	B-I
SN 2000fr
-0.32	-0.51 $\pm$ 0.12
14.70	-0.50 $\pm$ 0.24
29.08	1.42 $\pm$ 0.17
SN 1999ff
5.59	-0.18 $\pm$ 0.13
27.20	1.38 $\pm$ 0.24

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