In this activity, you will use data from various cosmological measurements in order to determine the values of several cosmological values: the amount of matter (Ω m ), which is comprised of regular b...In this activity, you will use data from various cosmological measurements in order to determine the values of several cosmological values: the amount of matter (Ω m ), which is comprised of regular baryonic matter and cold dark matter, and the amount of dark energy (Ω DE ). For a given source, the combination of Ω m and Ω DE has a 68% chance of falling within the smallest region, 95% chance of falling within the next larger region, and a 99% chance of falling within the entire shaded region.
