UCSB South Pole 1994 Cosmic Microwave Background Anisotropy Measurement Constraints on Open and Flat‐Λ Cold Dark Matter Cosmogonies

We develop methods to account for experimental and observational uncertainties in likelihood analyses of data from cosmic microwave background (CMB) anisotropy experiments and apply them to an analysis of the UCSB South Pole 1994 (SP94) experiment. Observationally motivated open and spatially at ", cold dark matter cosmogonies are considered. Among the models we consider, the full SP94 data set is most consistent with open models and less so with old Gyr), high