Dependence of cosmic shear covariances on cosmology - Impact on parameter estimation | A&A

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Table 2:

The ML-parameter sets which occur when choosing different starting cosmologies in the iterative likelihood analysis.
Step	run1		run2		run3		run4		run5
	$\Omega _{\rm m}$	${\sigma _8}$	$\Omega _{\rm m}$	${\sigma _8}$	$\Omega _{\rm m}$	${\sigma _8}$	$\Omega _{\rm m}$	${\sigma _8}$	$\Omega _{\rm m}$	${\sigma _8}$
${\vec \pi}_{\rm start}$	0.20	0.60	0.237	0.740	0.250	0.90	0.274	0.850	0.40	1.0
${\vec \pi}_{\rm ML}$ 1	0.254	0.892	0.254	0.892	0.245	0.914	0.259	0.884	0.277	0.858
${\vec \pi}_{\rm ML}$ 2	0.260	0.882	0.260	0.882	0.245	0.914	0.260	0.882	0.259	0.884
${\vec \pi}_{\rm ML}$ 3	0.260	0.882	0.260	0.882	converged		0.260	0.882	0.260	0.882
${\vec \pi}_{\rm ML}$ 4	converged		converged		converged		converged		0.260	0.882

Source LaTeX | All tables | In the text