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About

Ramon Miquel is a leading experimental cosmologist whose work is central to understanding the accelerating expansion of the universe. His primary research focuses on dark energy, galaxy clustering, and the cosmic distance scale, with a particular emphasis on measuring baryon acoustic oscillations (BAOs) to probe the universe’s large-scale structure. Miquel is a key member of the Dark Energy Spectroscopic Instrument (DESI) collaboration, where he contributed to the first detection of the BAO signal from early DESI data (37 citations), a milestone that demonstrated the instrument’s power to map the cosmos with unprecedented precision. This work, based on 261,291 luminous red galaxies, provided an early glimpse into DESI’s potential to constrain dark energy models. Beyond DESI, Miquel has made significant contributions to the Dark Energy Survey (DES) and other large-scale structure projects, helping to refine measurements of the Hubble constant and the matter density of the universe. His research has garnered thousands of citations, reflecting its profound impact on modern cosmology. Miquel’s ability to bridge theoretical predictions with cutting-edge observational data makes him a pivotal figure in the quest to understand dark energy.