Table 2: Best-fit parameters of the GRB 000911 host galaxy obtained with the Hyperz code. Photometric redshift errors are at 68% confidence level. The value of the luminosity $L^\star$ at the knee of the galaxies luminosity distribution (as defined by Schechter 1976; see Sect. 4.3) is taken from Lilly et al. (1995).
Template $\chi^2$ /d.o.f. Photometric Age $A_{\rm V}$ $M_{\rm B}$ $L/L^\star$

galaxy redshift (Gyr) (mag)

Irr-LMC 0.685 $\rm0.904^{+0.125}_{-0.128}$ 0.509 0.39 -18.40 0.066

Irr-Stb 0.731 $\rm0.904^{+0.134}_{-0.130}$ 0.509 0.55 -18.38 0.066

Irr-SMC 0.732 $\rm0.904^{+0.149}_{-0.138}$ 0.719 0.32 -18.37 0.064

**Table 2:** Best-fit parameters of the GRB 000911 host galaxy obtained with the *Hyperz* code. Photometric redshift errors are at 68% confidence level. The value of the luminosity $L^\star$ at the knee of the galaxies luminosity distribution (as defined by Schechter 1976; see Sect. 4.3) is taken from Lilly et al. (1995).
Template	$\chi^2$ /d.o.f.	Photometric	Age	$A_{\rm V}$	$M_{\rm B}$	$L/L^\star$
galaxy		redshift	(Gyr)	(mag)
Irr-LMC	0.685	$\rm0.904^{+0.125}_{-0.128}$	0.509	0.39	-18.40	0.066
Irr-Stb	0.731	$\rm0.904^{+0.134}_{-0.130}$	0.509	0.55	-18.38	0.066
Irr-SMC	0.732	$\rm0.904^{+0.149}_{-0.138}$	0.719	0.32	-18.37	0.064

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Results
	4 Discussion
	5 Conclusions
	References