Proceedings of the

The standard method for extracting cosmological parameters from the CMB is
through the use of Maximum Likelihood methods. In general the likelihood
function, , for a set of parameters, , is given by a
hypothesis, , for the distribution function of the data set. In the case
of uniform prior, and assuming a multivariate Gaussian distributed data set
consistent with Inflationary models, the * a posteriori* probability
distribution for the parameters is

where are the usual cosmological parameters we would like to determine. Examples of data are or and the statistics of the data are fully parametrised by the data covariance matrix, . For simplicity here we assume the data have zero means.

Fri Jun 20 15:22:24 BST 1997