Table 6: Summary of uncertainties in the derived cosmological parameters. The dominant systematic uncertainty arises from the photometric calibration, itself dominated by the $i_{\rm M}$ and $z_{\rm M}$ band contributions.
Source $\sigma(\Omega_{\rm M}$ ) $\sigma(\Omega_{\rm tot})$ $\sigma(w)$ $\sigma(\Omega_{\rm M})$ $\sigma(w)$

(flat) (with BAO)

Zero-points 0.024 0.51 0.05 0.004 0.040

Vega spectrum 0.012 0.02 0.03 0.003 0.024

Filter bandpasses 0.007 0.01 0.02 0.002 0.013

Malmquist bias 0.016 0.22 0.03 0.004 0.025

Sum ( sys) 0.032 0.55 0.07 0.007 0.054

Meas. errors 0.037 0.52 0.09 0.020 0.087

U-B color ( stat) 0.020 0.10 0.05 0.003 0.021

Sum ( stat) 0.042 0.53 0.10 0.021 0.090

**Table 6:** Summary of uncertainties in the derived cosmological parameters. The dominant systematic uncertainty arises from the photometric calibration, itself dominated by the $i_{\rm M}$ and $z_{\rm M}$ band contributions.
Source	$\sigma(\Omega_{\rm M}$ )	$\sigma(\Omega_{\rm tot})$	$\sigma(w)$	$\sigma(\Omega_{\rm M})$	$\sigma(w)$
	(flat)			(with BAO)
Zero-points	0.024	0.51	0.05	0.004	0.040
Vega spectrum	0.012	0.02	0.03	0.003	0.024
Filter bandpasses	0.007	0.01	0.02	0.002	0.013
Malmquist bias	0.016	0.22	0.03	0.004	0.025
Sum ( sys)	0.032	0.55	0.07	0.007	0.054
Meas. errors	0.037	0.52	0.09	0.020	0.087
U-B color ( stat)	0.020	0.10	0.05	0.003	0.021
Sum ( stat)	0.042	0.53	0.10	0.021	0.090

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