Dark-energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5

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Table 1:

Shear top-hat variance at 5' and 25' and for five redshift ranges. The error bars are Poisson noise.
	$\langle \vert\gamma^2(5\hbox{$^\prime$ })\vert \rangle/10^5$		$\langle \vert\gamma^2(25\hbox{$^\prime$ })\vert \rangle/10^5$
z-range	CFHTLS	prediction	CFHTLS	prediction
$0.0\phantom{0} \ldots 0.65$	$-0.3 \pm 2.0$	0.95	$0.2 \pm 0.5$	0.29
$0.0\phantom{0} \ldots 2.5$	$\phantom{-}1.9 \pm 0.9$	2.38	$0.7 \pm 0.2$	0.73
$0.65 \ldots 0.95$	$\phantom{-}2.9 \pm 2.2$	4.12	$1.1 \pm 0.5$	1.27
$0.65 \ldots 2.5$	$\phantom{-}3.3 \pm 1.4$	4.77	$0.9 \pm 0.3$	1.48
$0.95 \ldots 2.5$	$-1.7 \pm 3.7$	7.46	$0.04 \pm 0.9$	2.33

Source LaTeX | All tables | In the text

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