Using weak lensing to find halo masses
Authors:
- Roland de PutterRPRoland de Putter
- Martin WhiteMWMartin White
- 31 August 2005
- journal article
- Published by Elsevier in New Astronomy
- Vol. 10 (8) , 676-687
Abstract
No abstract availableKeywords
All Related Versions
This publication has 23 references indexed in Scilit:
- Shear‐selected Cluster Cosmology: Tomography and Optimal FilteringThe Astrophysical Journal, 2005
- The Dark Side of the Halo Occupation DistributionThe Astrophysical Journal, 2004
- A Merged Catalog of Clusters of Galaxies from Early Sloan Digital Sky Survey DataThe Astrophysical Journal Supplement Series, 2003
- Profiles of dark haloes: evolution, scatter and environmentMonthly Notices of the Royal Astronomical Society, 2001
- Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass FunctionsThe Astrophysical Journal, 2000
- A New Algorithm for Computing Statistics of Weak Lensing by Large‐Scale StructureThe Astrophysical Journal, 2000
- Weak Lensing by Large-Scale Structure: A Dark Matter Halo ApproachThe Astrophysical Journal, 2000
- Ray‐tracing Simulations of Weak Lensing by Large‐Scale StructureThe Astrophysical Journal, 2000
- Power Spectra for Cold Dark Matter and Its VariantsThe Astrophysical Journal, 1999
- The evolution of large-scale structure in a universe dominated by cold dark matterThe Astrophysical Journal, 1985