Four microwave telescopes at the South Pole will search the CMB for evidence of cosmic inflation, a popular theory of the universe’s first fraction of a second of existence.

CMB-S4’s microwave telescopes at the South Pole and Chile’s Atacama Plateau will search the sky for evidence of primordial gravitational waves, a sign of inflation.

Fermi’s Large Area Telescope will perform a continuous, all-sky survey to study a range of astrophysical phenomena, including indirect searches for dark matter.

Located deep underground, the SuperCDMS collaboration is searching for dark matter particles with masses smaller than ten times the mass of the proton.

LZ searches for dark matter by looking for collisions with xenon nuclei inside a tank of purified xenon 4,850 feet underground in South Dakota's Sanford Underground Research Facility.

DES studies dark energy through its impact on the abundance of galaxy clusters, gravitational lensing, supernovae and detections of large-scale correlations between galaxies.

LSST will take images of the entire visible southern sky over and over for a decade, creating a vast, public archive of data that will dramatically advance our knowledge of dark energy and dark matter.

KIPAC brings the power of theory, computation, experiments and observations to bear on astrophysical questions, from the origins of cosmic rays to the structure and evolution of the universe.

SLAC's Computational Astrophysics group seeks to bring the combined strength of theoretical and experimental physics to bear on some of the most fascinating problems in particle astrophysics and cosmology.

KIPAC's visualization and data analysis facilities help scientists at KIPAC and SLAC analyze their large-scale scientific data sets, including building stunning visual recreations of the evolution of the universe