Theoretical implications of microwave background radiation anisotropy experiments
arXiv:astro-ph/9611228
Abstract
Observational results from several experiments such as COBE, SP, Saskatoon, PYTHON, ARGO, MAX, MSAM, Tenerife and CAT are considered and a comparison is made with predictions from several models. Conclusions are reached about the viability of current structure formation models.
7 pages LaTeX, including 6 PostScript figures. To appear in proceedings of the XXXIst Rencontre de Moriond, `Microwave Background Anisotropies'