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About

G. Dhungana is a key contributor to the Dark Energy Spectroscopic Instrument (DESI) collaboration, focusing on the instrumentation and data analysis that underpin one of the most ambitious cosmological surveys ever undertaken. Their work centers on understanding dark energy through precise spectroscopic measurements of 40 million galaxies and quasars, employing the Baryon Acoustic Oscillation technique to map the universe’s expansion history. Dhungana’s most cited paper, the 2022 DESI instrumentation overview, has already garnered 10 citations, reflecting its foundational role in the project. This work details the complex engineering and calibration required to achieve the survey’s unprecedented redshift accuracy. Beyond instrumentation, Dhungana’s contributions to DESI’s data processing pipelines and early science results are helping to refine our models of cosmic structure formation. Their efforts are critical to the survey’s five-year mission, which promises to deliver transformative insights into the nature of dark energy and the large-scale structure of the cosmos.