Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
Kavli Institute for Particle Astrophysics and Cosmology · Stanford University · +68 more institutions
Abstract
This work, together with its companion paper, Secco, Samuroff et al. [Phys. Rev. D 105, 023515 (2022)], present the Dark Energy Survey Year 3 cosmic-shear measurements and cosmological constraints based on an analysis of over 100 million source galaxies. With the data spanning $4143\text{ }\text{ }{\mathrm{deg}}^{2}$ on the sky, divided into four redshift bins, we produce a measurement with a signal-to-noise of 40. We conduct a blind analysis in the context of the Lambda-Cold Dark Matter ($\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$) model and find a 3% constraint of the clustering amplitude,…
Citation impact
- FWCI
- 58.20
- Percentile
- 100%
- References
- 230
Authors
147- AAA. AmonCorresponding
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
- DGD. Gruen
SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
- MAM. A. Troxel
Duke University
- NMN. MacCrann
University of Cambridge
- SDScott Dodelson
Carnegie Mellon University
Topics & keywords
- Physics
- Cosmic microwave background
- Redshift
- Astrophysics
- Dark energy
- Galaxy
- Cosmology
- Planck
- Affordable and clean energy
Funding
- NSNational Science FoundationAwards: ESP2017-89838, PGC2018-102021, 1536171, SEV-2016-0588, 2012B-0001, AST-1536171, SEV-2016-0597, DE-AC02-07CH11359, PGC2018-094773, MDM-2015-0509, 1138766, AST-1138766
- UDU.S. Department of EnergyAwards: DE-AC02-07CH11359, AC02-07CH11359, DE-AC02, DE-AC02-
- NANational Aeronautics and Space Administration
- UOUniversity of Pennsylvania
- OSOhio State University
- UOUniversity of Chicago
- TATexas A and M University
- UOUniversity of Portsmouth
- NCNational Centre for Supercomputing Applications
- HEHigher Education Funding Council for England
- CDCentres de Recerca de Catalunya
- UCUniversity College London
- ECEuropean CommissionAwards: 306478, 240672, 291329, 2007-2013
- UOUniversity of Sussex
- DFDeutsche ForschungsgemeinschaftAwards: DE-AC02-07CH11359, SEV-2016-0597, AST-1536171, AST-1138766
- GDGeneralitat de Catalunya
- MDMinistério da Ciência, Tecnologia e Inovação
- CNConselho Nacional de Desenvolvimento Científico e TecnológicoAwards: SEV-2016-0597, /2014-2, 2014-2, 465376/2014-2
- FCFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
- FDFinanciadora de Estudos e Projetos
- MDMinisterio de Ciencia e InnovaciónAwards: ESP2017-89838, MDM-2015-0509, PGC2018-102021, PGC2018, PGC2018-094773, SEV-2016-0597, SEV-2016-0588
- IDInstitut de Física d'Altes Energies
- UOUniversity of Illinois at Urbana-Champaign
- OOOffice of ScienceAwards: DE-AC02, DE-AC02-07CH11359
- SFSeventh Framework Programme
- CFCenter for Cosmology and Astroparticle Physics, Ohio State University
- SAScience and Technology Facilities CouncilAwards: ST/P000525/1, DE-AC02-07CH11359, ST/S000550/1, ST/R000972/1, ST/T000473/1, ST/T003081/1, ST/T000414/1, ST/N001087/1, ST/M003574/1
- EREuropean Research CouncilAwards: 240672, 306478, 291329
- EREuropean Regional Development FundAwards: SEV-2016-0588, PGC2018-102021, 240672, MDM-2015-0509, 291329, ESP2017-89838, 2007-2013, 306478, SEV-2016-0597, PGC2018-094773, PGC2018
- CDCentro de Investigaciones Energéticas, Medioambientales y TecnológicasAward: MDM-2015-0509
- HEHigh Energy Physics
- IEIntegrated Electronics Engineering Center, Binghamton University
- ANArgonne National LaboratoryAward: DE-AC02
- FFermilab
- LBLawrence Berkeley National LaboratoryAward: DE-AC02-07CH11359
- SNSLAC National Accelerator Laboratory