Table 5: Summary of IR data for SN 1999ff. Epochs are in restframe days relative to the date of the B-band maximum ( $t_{\rm max}={\rm MJD}~51494.8$ ); restframe I-band magnitudes are computed applying k-corrections to the observed J-band data published in Tonry et al. (2003). The uncertainties also include the contribution from k-corrections, estimated to be 0.05 mag at all epochs considered.
$\rm MJD$ Epoch I(mag)

51501.29 5.01 23.57 $\pm$ 0.11

51526.31 22.21 24.06 $\pm$ 0.24

**Table 5:** Summary of IR data for SN 1999ff. Epochs are in restframe days relative to the date of the B-band maximum ( $t_{\rm max}={\rm MJD}~51494.8$ ); restframe I-band magnitudes are computed applying k-corrections to the observed J-band data published in Tonry et al. (2003). The uncertainties also include the contribution from k-corrections, estimated to be 0.05 mag at all epochs considered.
$\rm MJD$	Epoch	I(mag)
51501.29	5.01	23.57 $\pm$ 0.11
51526.31	22.21	24.06 $\pm$ 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