Facilities for Dark Energy Investigations

Abstract

The discovery of cosmic acceleration has inspired ambitious experimental and observational efforts to understand its origin. Many of these take the form of large astronomical surveys, sometimes using new, special-purpose instrumentation, and in some cases entirely new facilities. This Report summarizes some of the major ongoing and planned dark energy experiments, focusing on those in which the U.S. community has a leading or significant supporting role. It provides background information for other Reports from the "Dark Energy and CMB" working group of the APS Division of Particles and Fields long-term planning exercise. We provide 1-2 page summaries of the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) and its SDSS-IV successor eBOSS, the Dark Energy Survey (DES), the Subaru Hyper-Suprime Camera (HSC) and Prime Focus Spectrograph (PFS), the Hobby-Eberley Telescope Dark Energy Experiment (HEDTEX), the Dark Energy Spectroscopic Instrument (DESI), the Large Synpotic Survey Telescope (LSST), and the Euclid and AFTA-WFIRST (Wide Field Infrared Survey Telescope) space missions. Over the next one to two decades, these experiments seek to improve the precision of measurements of the cosmic expansion history and cosmic structure growth by factors of 10-100, while simultaneously increasing their redshift range and tightening control and cross-checks of sytematic effects. These measurements will dramatically improve the empirical constraints on theoretical explanations of cosmic acceleration and could lead to breakthroughs in our understanding of the nature of gravity and spacetime or the forms of energy present in the universe.