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Version 7 (Shantanu Desai, 10/25/2012 10:21 AM) → Version 8/17 (Jörg Dietrich, 10/25/2012 12:00 PM)

h1. Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts

We make the first detailed MCMC likelihood study of cosmological constraints that are expected from some of the largest, ongoing and proposed, cluster surveys in different wave-bands and compare the estimates to the prevalent Fisher matrix forecasts.
http://arxiv.org/pdf/1210.5586v1.pdf

h2. Star-Galaxy Classification in Multi-Band Optical Imaging.

Ground-based optical surveys such as PanSTARRS, DES, and LSST, will produce large catalogs to limiting magnitudes of r > 24. Star-galaxy separation poses a major challenge to such surveys because galaxies---even very compact galaxies---outnumber halo stars at these depths
http://arxiv.org/abs/1206.4306

h2. The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars

We measure the cross-correlation of Atacama Cosmology Telescope CMB lensing convergence maps with quasar maps made from the Sloan Digital Sky Survey DR8 SDSS-XDQSO photometric catalog.
http://arxiv.org/abs/1207.4543

h2. CALCLENS: Weak Lensing Simulations for Large-area Sky Surveys and Second-order Effects in Cosmic Shear Power Spectra

http://arxiv.org/abs/1210.3069
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