22-26 August 2011, Porto, Portugal
Bayesian reconstruction of the gravitational potential from weak lensing Mass mapping using weak lensing has been a very successful technique in cosmology as proven by the indication of a Dark Matter component in the Bullet Cluster. In addition, if combined with information from clustering and peculiar velocities, it can be a promising probe of Dark Energy and Modified Gravity. Here, I review the Bayesian approaches to weak lensing potential reconstruction and propose a Maximum-Probability method. I discuss how to incorporate prior information in the reconstruction process of 2D and 3D maps of the gravitational potential due to large scale structure and show the results of applying this method to N-body simulations. |
We use cookies to ensure that you get the best experience on our website, by continuing on this website you agree to the storing of cookies on your device. Learn more about our Privacy Policy .