Table 4: Summary of $J_{\rm s}$ -band data for SN 2000fr. The quoted errors are due to statistical Poisson noise and the uncertainty in the ZP (contributing 0.01 mag). Epochs are in restframe days relative to the date of B-band maximum. The restframe I-band is obtained through cross-filter k-correction from the observed $J_{\rm s}$ -band to Bessel I-band. The uncertainties also include the contribution from k-corrections, estimated to be 0.05 mag at all epochs considered.
MJD Epoch $J_{\rm s}$ (mag) I(mag)

51685.06 -0.33 22.50 $\pm$ 0.09 23.52 $\pm$ 0.10

51709.02 15.20 23.57 $\pm$ 0.22 24.52 $\pm$ 0.23

51731.96 30.07 23.14 $\pm$ 0.15 23.99 $\pm$ 0.16

**Table 4:** Summary of $J_{\rm s}$ -band data for SN 2000fr. The quoted errors are due to statistical Poisson noise and the uncertainty in the ZP (contributing 0.01 mag). Epochs are in restframe days relative to the date of B-band maximum. The restframe I-band is obtained through cross-filter k-correction from the observed $J_{\rm s}$ -band to Bessel I-band. The uncertainties also include the contribution from k-corrections, estimated to be 0.05 mag at all epochs considered.
MJD	Epoch	$J_{\rm s}$ (mag)	I(mag)
51685.06	-0.33	22.50 $\pm$ 0.09	23.52 $\pm$ 0.10
51709.02	15.20	23.57 $\pm$ 0.22	24.52 $\pm$ 0.23
51731.96	30.07	23.14 $\pm$ 0.15	23.99 $\pm$ 0.16

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