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Likelihood Analysis of Galaxy Surveys
Scott Dodelson, Lam Hui, Andrew Jaffe
One of the major goals of cosmological observations is to test theories of structure formation. The most straightforward way to carry out such tests is to compute the likelihood fu…
Bending of Light by Vector Perturbations
S. Dodelson, C. Wiegert
A number of different mechanisms exist which can produce vector perturbations to the metric. One might think that such perturbations could deflect light rays from distant sources,…
On the Computation of CMBR Anisotropies from Simulations of Topological Defects
Albert Stebbins, Scott Dodelson
Techniques for computing the CMBR anisotropy from simulations of topological defects are discussed with an eye to getting as much information from a simulation as possible. Here we…
Anisotropies in the Cosmic Microwave Background: Theory
Scott Dodelson
Anisotropies in the Cosmic Microwave Background (CMB) contain a wealth of information about the past history of the universe and the present values of cosmological parameters. I ou…