2011/11/28 by Adrienne Leonard, François-Xavier Dupé, Jean-Luc Starck +1
Engineering · Mathematics · Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy #Astrophysics #Context (archaeology) #Cosmology #Distribution (mathematics) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geography #Gravitation #Gravitational lens #Gravitational lensing formalism #Ideal (ethics) #Mass distribution #Mathematical analysis #Mathematics #Physics #Redshift #Sparse and Compressive Sensing Techniques #Strong gravitational lensing #Universe #Weak gravitational lensing #astro-ph.CO
paper · pdf · doi:10.1051/0004-6361/201117642
Submitted to A&A (6 July 2011)
arxiv created 2011/11/28 · openalex publication_date 2011/12/16 · arxiv updated 2015/06/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context. Weak gravitational lensing is an ideal probe of the dark universe. In recent years, several linear methods have been developed to reconstruct the density distribution in the Universe in three dimensions, making use of photometric redshift information to determine the radial distribution of lensed sources.