Dec 13 – 18, 2015
International Conference Centre Geneva
Europe/Zurich timezone

CMB lensing - galaxy cross-correlations

Dec 17, 2015, 3:24 PM
Level -1, Room 16 (International Conference Centre Geneva)

Level -1, Room 16

International Conference Centre Geneva

17 Rue de Varembé, 1211 Geneva


Mr Yuuki Omori (McGill University)


Large scale structure in the universe causes gravitational lensing of the cosmic microwave background (CMB), which has now been well-measured by several CMB experiments. By cross-correlating CMB lensing with tracers of large scale structure (like galaxies), it is possible to obtain new constraints on cosmology and a better understanding of possible systematic errors in cosmological probes. I will discuss the theoretical formulation, methods used in estimating errors, systematic checks to verify robustness, and cosmological implications of cross-correlations between CMB lensing and galaxy surveys, and will present recent results of cross-correlation analyses.
Collaboration SPT & DES collaborations

Primary author

Mr Yuuki Omori (McGill University)

Presentation materials