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Weak Lensing: Prospects for Measuring Cosmological Parameters
Wayne Hu, Max Tegmark
Weak lensing of galaxies by large scale structure can potentially measure cosmological quantities as accurately as the cosmic microwave background (CMB). However, the relation betw…
Bias and beyond
Max Tegmark
It is becoming increasingly clear that galaxy bias is complicated, with evidence indicating that it can be time-dependent, morphology-dependent, scale-dependent, non-linear and non…
Cosmic complementarity: combining CMB and supernova observations
Max Tegmark, Daniel J. Eisenstein, Wayne Hu
We compute the accuracy with which Omega and Lambda can be measured by combining future SN Ia and CMB experiments, deriving a handy expression for the SN Ia Fisher information matr…
The time-evolution of bias
Max Tegmark, P. J. E. Peebles
We study the evolution of the bias factor b and the mass-galaxy correlation coefficient r in a simple analytic model for galaxy formation and the gravitational growth of clustering…