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If you have a question about this talk, please contact Martin Haehnelt. The ongoing Cosmic Microwave Background (CMB) polarization experiment POLARBEAR and its upgrade, the Simons Array, will provide one of the best CMB data sets for both cosmological applications and CMB -galaxy surveys cross-correlation studies. In this talk I will review the latests results and data analysis activity of POLARBEAR and outline the capabilities of the Simons array to constrain cosmology and capitalize on cross-correlation analyses. If time allows, I will also discuss both the challenges encountered when modeling jointly CMB and Large-Scale Structure distribution and recent numerical results trying to address these issues for the current and future generation of experiments. This talk is part of the Galaxies Discussion Group series. This talk is included in these lists:
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