Table 9: Restframe B-V colours in magnitudes for SN 1999ff and SN 2000fr. The Epoch is in rest frame days relative to the B-band maximum, divided by the B-band stretch.
Epoch B-V
SN 2000fr  
-7.97 -0.06 $\pm $ 0.05a
-3.51 -0.14 $\pm $ 0.05a
4.60 -0.12 $\pm $ 0.05
12.93 0.24 $\pm $ 0.08
20.31 0.61 $\pm $ 0.07
30.22 0.99 $\pm $ 0.09
SN 1999ff  
-7.99 0.03 $\pm $ 0.08a
1.91 -0.02 $\pm $ 0.09
1.98 0.10 $\pm $ 0.12
2.91 0.23 $\pm $ 0.12
19.55 0.71 $\pm $ 0.09
28.75 1.22 $\pm $ 0.20
a The data are not included in the analysis because they are out of the range
in which Nobili et al. (2003) studied colour correlations.

Source LaTeX | All tables | In the text

Article Contents
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
List of tables
List of figures