The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set
Institut d'Astrophysique de Paris · Laboratoire de Physique Subatomique et de Cosmologie · +2 more institutions
Abstract
Abstract We present cosmological constraints from the sample of Type Ia supernovae (SNe Ia) discovered and measured during the full 5 yr of the Dark Energy Survey (DES) SN program. In contrast to most previous cosmological samples, in which SNe are classified based on their spectra, we classify the DES SNe using a machine learning algorithm applied to their light curves in four photometric bands. Spectroscopic redshifts are acquired from a dedicated follow-up survey of the host galaxies. After accounting for the likelihood of each SN being an SN Ia, we find 1635 DES SNe in the redshift range 0.10 < z < 1.13 that pass quality selection criteria sufficient to constrain cosmological parameters. This…
Citation impact
- FWCI
- 108.26
- Percentile
- 100%
- References
- 148
Authors
157Topics & keywords
- Redshift
- Supernova
- Physics
- Dark energy
- Astrophysics
- Cosmology
- Type (biology)
- Galaxy
- Affordable and clean energy
Funding
- NSNational Science FoundationAwards: 1518052, ESP2017-89838, AST-1518052, PGC2018-102021, 1536171, SEV-2016-0588, 2012B-0001, AST-1815935, FP7/2007-2013, AST-1536171, SEV-2016-0597, DE-AC02-07CH11359, PGC2018-094773, AST-2108094, 2108094, MDM-2015-0509, DE-AC02-05CH11231, NAS 5-26555, 1138766, AST-1138766
- UDU.S. Department of EnergyAwards: -AC02-05CH11231, DE-FOA-0002424, DE-AC02-07CH11359, 05CH11231, DE-SC0009924, AC02-07CH11359, AC02-05CH11231, DE-AC02, NAS 5-26555, DE-AC02-05CH11231, -7887, DE-AC02-
- NANational Aeronautics and Space AdministrationAwards: DE-AC02-05CH11231, MR/T01881X/1, HST-HF2-51546.001-A, NAS5-26555, 14-WPS14-0048, NNG16PJ34G, NAS 5-26555, 5-26555, NNG17PX03C, AR-14296
- APAlfred P. Sloan FoundationAward: DE-AC02-05CH11231
- WMW. M. Keck Foundation
- GAGordon and Betty Moore Foundation
- UOUniversity of Pennsylvania
- OSOhio State University
- CICalifornia Institute of Technology
- UOUniversity of ChicagoAward: NAS 5-26555
- UOUniversity of Michigan
- UOUniversity of PortsmouthAward: NAS 5-26555
- STSpace Telescope Science InstituteAwards: NAS5-26555, NAS 5-26555, 5-26555, 26555
- URUK Research and InnovationAward: MR/T01881X/1
- CDCentres de Recerca de CatalunyaAward: 501100011033
- AGAustralian GovernmentAwards: DE230100055, FL180100168
- NENational Energy Research Scientific Computing CenterAwards: 05CH11231, HEP-ERCAP0023923, AC02-05CH11231
- UCUniversity College London
- ECEuropean CommissionAwards: 306478, 240672, 10.13039/501100011033, 13039/501100011033, FP7/2007-2013, 291329, 501100011033, DE-AC02-05CH11231, 2007-2013, FP7/2007, PID2020-115253GA-I00
- UOUniversity of Nottingham
- UOUniversity of Sussex
- DFDeutsche ForschungsgemeinschaftAwards: DE-AC02-07CH11359, DE-AC02-05CH11231, SEV-2016-0597, FP7/2007-2013, NAS 5-26555, AST-1536171, AST-1138766
- GDGeneralitat de CatalunyaAwards: 10.13039/501100011033, 501100011033, CEX2020-001058-M
- MDMinistério da Ciência, Tecnologia e Inovação
- CNConselho Nacional de Desenvolvimento Científico e TecnológicoAwards: SEV-2016-0597, 2014-2, 465376/2014-2
- KAKorea Astronomy and Space Science Institute
- 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, 10.13039, CEX2020-001058-M, MDM-2015-0509, PGC2018-102021, PGC2018, 501100011033, PID2020, PID2020-, PGC2018-094773, 10.13039/501100011033, SEV-2016-0597, 13039/501100011033, SEV-2016-0588, PID2020-115253GA-I00
- MDMinistério da Ciência, Tecnologia, Inovações e Comunicações
- ANAgencia Nacional de Investigación y Desarrollo
- IDInstitut de Física d'Altes Energies
- UOUniversity of Illinois at Urbana-ChampaignAward: 13039
- OOOffice of ScienceAwards: AC02-05CH11231, -AC02-05CH11231, DE-AC02, DE-AC02-07CH11359
- SAScience and Technology Facilities CouncilAwards: DE-AC02-07CH11359, FP7/2007-2013, CEX2020-001058-M, ST/X001229/1
- EREuropean Regional Development FundAwards: SEV-2016-0588, PGC2018-102021, 240672, MDM-2015-0509, CEX2020-001058-M, DE-AC02-05CH11231, 291329, ESP2017-89838, 2007-2013, 10.13039/501100011033, 13039/501100011033, FP7/2007-2013, 501100011033, 306478, SEV-2016-0597, PGC2018-094773, PGC2018
- AEAgencia Estatal de InvestigaciónAwards: SEV-2016-0597, 501100011033, PID2020-115253GA-I00, 10.13039/501100011033, CEX2020-001058-M, 13039, 10.13039, 13039/501100011033, SEV-2016-0588
- HEHigh Energy PhysicsAwards: DE-SC0009924, DE-AC02-05CH11231
- IEIntegrated Electronics Engineering Center, Binghamton University
- ESEuropean Social FundAwards: FP7/2007-2013, 2007-2013, 501100011033, RYC2019-027683-I, CEX2020-001058-M, PID2020-115253GA-I00
- ANArgonne National LaboratoryAwards: DE-AC02, DE-AC02-05CH11231
- FFermilabAward: NAS 5-26555
- LBLawrence Berkeley National LaboratoryAwards: DE-AC02-05CH11231, DE-AC02-07CH11359, 05CH11231, AC02-05CH11231
- SNSLAC National Accelerator LaboratoryAward: DE-AC02-05CH11231