Dark Energy Survey Year 3 results: Simulation-based cosmological inference with wavelet harmonics, scattering transforms, and moments of weak lensing mass maps. II. cosmological results
M. GattiUniversity of PennsylvaniaG. CampaillaMIT, Cambridge, Dept. PhysN JeffreyUniversity College LondonL WhitewayUniversity College LondonA. PorredonRuhr University BochumJ. PratUniversity of ChicagoJ. WilliamsonUniversity College LondonM RaveriMIT, Cambridge, Dept. PhysBhuvnesh JainUPenn, PhiladelphiaVirginia AjaniChicago U., Astron. Astrophys. CtrG. GianniniUniversity of ChicagoM. YamamotoDuke University DurhamConghao ZhouSanta Cruz Institute for Particle PhysicsJ BlazekNortheastern UniversityDhayaa AnbajaganeUniversity of ChicagoS. SamuroffNortheastern UniversityTomasz KacprzakETH ZurichA. AlarconArgonne National LaboratoryA. AmonCambridge U., KICCK. BechtolUniversity Avenue MadisonM. R. BeckerArgonne National LaboratoryG. M. BernsteinUniversity of PennsylvaniaA. CamposUniversity Avenue MadisonC. ChangChicago U., KICPR. ChenDuke University DurhamA. ChoiNASA Goddard Space Flight CenterC. DavisStanford UniversityJ. DeRoseLawrence Berkeley National LaboratoryH. T. DiehlFermi National Accelerator LaboratoryScott DodelsonCarnegie Mellon UniversityC. DouxUniversité Grenoble AlpesK. EckertUPenn, PhiladelphiaJ. Elvin-PooleWaterloo US. EverettCalifornia Institute of TechnologyA. FertéSLAC National Accelerator LaboratoryD. GruenUniversity ObservatoryR. A. GruendlCenter for Astrophysical SurveysI. HarrisonCardiff UniversityW G HartleyUniversity of GenevaK. HernerFermi National Accelerator LaboratoryE. M. HuffCalifornia Institute of TechnologyMike JarvisUniversity of PennsylvaniaN. KuropatkinFermi National Accelerator LaboratoryP.-F. LégetStanford UniversityN. MacCrannUniversity of CambridgeJ. McCulloughStanford UniversityJ. MylesPrinceton UniversityA Navarro-AlsinaUniversidade Estadual de CampinasS. PandeyUniversity of PennsylvaniaR. P. RollinsJodrell BankA. RoodmanStanford UniversityC. SánchezUniversity of PennsylvaniaL. F. SeccoUniversity of ChicagoI. Sevilla-NoarbeMedioambientales y Tecnológicas (CIEMAT)E. SheldonBrookhavenT. ShinStony Brook UniversityM. A. TroxelDuke University DurhamI. TutusausUniversité de ToulouseT. N. VargaMax Planck Institute for Extraterrestrial PhysicsB. YannyFermi National Accelerator LaboratoryB. YinCarnegie Mellon UniversityY. ZhangCerro-Tololo InterAmerican ObsJ. ZuntzEdinburgh U., Inst. AstronT. AbbottCerro-Tololo InterAmerican ObsM. AguenaLaboratório Interinstitucional de e-Astronomia—LIneAS. S. AllamFermi National Accelerator LaboratoryO. AlvesU. Michigan, Ann ArborF. Andrade-OliveiraU. Michigan, Ann ArborD. BaconUniversity of PortsmouthS. BocquetUniversity ObservatoryDavid H. BrooksUniversity College LondonA. Carnero RosellInstituto de Astrofisica de CanariasJ. CarreteroBarcelona, IFAEL. N. da CostaLaboratório Interinstitucional de e-Astronomia—LIneAM. E. S. PereiraUniversität HamburgJ. De VicenteMadrid, CIEMATI. FerreroInstitute of Theoretical AstrophysicsJ. FriemanUniversity of ChicagoJ. García-BellidoUniversidad Autonoma de MadridE. GaztañagaUniversity of PortsmouthG. GutiérrezFermi National Accelerator LaboratoryS. R. HintonUniversity of QueenslandD. L. HollowoodUC, Santa CruzK. HonscheidOhio State UD.J JamesCenter for Astrophysics | Harvard & SmithsonianK. KuehnLowell ObservatoryO. LahavUniversity College LondonS. LeeCalifornia Institute of TechnologyJ. L. MarshallTexas A-MJ. Mena-FernándezLPSC Grenoble—53R. MiquelBarcelona, IFAEA. PieresRio de Janeiro ObservA. A. Plazas MalagónStanford UniversityE. SánchezMedioambientales y Tecnológicas (CIEMAT)D. Sanchez CidMadrid, CIEMATM. SchubnellUniversity of MichiganM SmithUniversity of SouthamptonE. SuchytaOak Ridge National LaboratoryG. TarléUniversity of MichiganN. WeaverdyckLBL, Berkeley
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The paper applies a novel simulation-based cosmological inference methodology to Dark Energy Survey Year-3-based weak-lensing mass maps. Inclusion of nongaussian statistics strongly improves cosmological constraints, establishing consistency with other work with the same and different datasets.
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