Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
NSF NOIRLab · Lawrence Berkeley National Laboratory · +88 more institutions
Abstract
Abstract The Dark Energy Spectroscopic Instrument (DESI) embarked on an ambitious 5 yr survey in 2021 May to explore the nature of dark energy with spectroscopic measurements of 40 million galaxies and quasars. DESI will determine precise redshifts and employ the baryon acoustic oscillation method to measure distances from the nearby universe to beyond redshift z > 3.5, and employ redshift space distortions to measure the growth of structure and probe potential modifications to general relativity. We describe the significant instrumentation we developed to conduct the DESI survey. This includes: a wide-field, 3.°2 diameter prime-focus corrector; a focal plane system with 5020 fiber positioners on the 0.812…
Citation impact
- FWCI
- 134.16
- Percentile
- 100%
- References
- 101
Authors
269Topics & keywords
- Physics
- Dark energy
- Instrumentation (computer programming)
- Redshift
- Telescope
- First light
- Galaxy
- Optics
- Affordable and clean energy
Funding
- NSNational Science FoundationAwards: No. AST-0950945, AST-0950945, DE-AC02-05CH11231, 0950945
- UDU.S. Department of EnergyAwards: -AC02-05CH11231, 05CH11231, No. DE-AC02-05CH11231, AC02-05CH11231, DE-AC02, DE-AC02-05CH11231, DE-AC02-
- GAGordon and Betty Moore Foundation
- YUYale UniversityAward: DE-AC02-05CH11231
- UOUniversity of Pennsylvania
- OSOhio State University
- HUHarvard University
- AUAix-Marseille Université
- UOUniversity of Pittsburgh
- CMCarnegie Mellon University
- UOUniversity of Rochester
- UOUniversity of Wyoming
- UOUniversity of Portsmouth
- HFHeising-Simons Foundation
- NENational Energy Research Scientific Computing CenterAwards: 05CH11231, AC02-05CH11231
- SMSouthern Methodist University
- ESEuropean Space Agency
- YUYork University
- UCUniversity College London
- DUDurham University
- ÉPÉcole Polytechnique Fédérale de Lausanne
- SUSwinburne University of Technology
- CNConsejo Nacional de Ciencia y Tecnología
- UOUniversity of Toronto
- KAKorea Astronomy and Space Science Institute
- UOUniversity of Waterloo
- MDMinisterio de Ciencia e Innovación
- SJShanghai Jiao Tong University
- UDUniversitat de Barcelona
- UZUniversität Zürich
- CÀCommissariat à l'Énergie Atomique et aux Énergies Alternatives
- IPInstitut Périmètre de physique théorique
- OOOffice of ScienceAwards: AC02-05CH11231, -AC02-05CH11231, DE-AC02, No. DE-AC02-05CH11231
- UOUniversity of California, Irvine
- SAScience and Technology Facilities CouncilAwards: ST/T005009/2, ST/W001225/1, ST/M002675/1, ST/M00287X/1
- DODivision of Astronomical SciencesAward: AST-0950945
- HEHigh Energy PhysicsAward: DE-AC02-05CH11231
- ANArgonne National LaboratoryAwards: DE-AC02, DE-AC02-05CH11231
- FFermilab
- BNBrookhaven National LaboratoryAward: DE-AC02-05CH11231
- LBLawrence Berkeley National LaboratoryAwards: DE-AC02-05CH11231, No. DE-AC02-05CH11231, 05CH11231, AC02-05CH11231
- SNSLAC National Accelerator LaboratoryAward: DE-AC02-05CH11231