Ricard Casas

TL;DR: DESI as discussed by the authors is a ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey.

TL;DR: The DESI Legacy Imaging Surveys project as discussed by the authors is a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image approximately 14,000 deg^2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory.

TL;DR: The DESI Legacy Imaging Surveys (http://legacysurvey.org/) as mentioned in this paper is a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ≈14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory.

TL;DR: In this article, a large multi-wavelength campaign was organized by the Whole Earth Blazar Telescope (WEBT) to follow the emission behavior of the radio quasar 3C 454.3.

TL;DR: In this paper, the authors present validated Euclid cosmological forecasts for galaxy clustering, weak lensing, and the combination thereof, which combine both theoretical and observational ingredients for different Cosmological probes.