http://arxiv.org/abs/1406.7796
We study the statistical inference of the cosmological dark matter density field from non-Gaussian, non-linear and non-Poisson biased distributed tracers. We have implemented a Bayesian posterior sampling computer-code solving this problem and tested it with mock data based on N-body simulations.
M. Ata, F. Kitaura and V. Muller
Tue, 1 Jul 14
42/70
Comments: Proceedings of IAU 306 Symposium, Statistical Challenges of the 21st Century Cosmology
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