SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos
S. BocquetLudwig-Maximilians-UniversitätS. GrandisLudwig-Maximilians-UniversitätL. E. BleemArgonne National LaboratoryMatthias KleinLudwig-Maximilians-UniversitätJ. J. MohrLudwig-Maximilians-UniversitätT. SchrabbackUniversität InnsbruckT. M. C. AbbottNSF’s National Optical-Infrared Astronomy Research LaboratoryP. A. R. AdeCardiff UniversityM. AguenaLaboratório Interinstitucional de e-Astronomia—LIneAA. AlarconArgonne National LaboratoryS. AllamFermi National Accelerator LaboratoryS. W. AllenSLAC National Accelerator LaboratoryO. AlvesUniversity of MichiganA. AmonUniversity of CambridgeA. J. AndersonFermi National Accelerator LaboratoryJ. AnnisFermi National Accelerator LaboratoryB. AnsarinejadUniversity of MelbourneJason E. AustermannUniversity of ColoradoS. ÀvilaInstitute of Science and TechnologyD. BaconUniversity of PortsmouthM. BaylissUniversity of CincinnatiJ. A. BeallNIST Quantum Devices GroupK. BechtolUniversity of Wisconsin-MadisonM. R. BeckerArgonne National LaboratoryA. N. BenderUniversity of ChicagoB. A. BensonFermi National Accelerator LaboratoryG. M. BernsteinUniversity of PennsylvaniaS BhargavaUniversity of SussexF. BianchiniStanford UniversityM. BrodwinUniversity of MissouriDavide BianchiUniversity College LondonLincoln BryantUniversity of ChicagoA. CamposCarnegie Mellon UniversityR. E. A. CanningUniversity of PortsmouthJ. E. CarlstromUniversity of ChicagoA. Carnero RosellLaboratório Interinstitucional de e-Astronomia—LIneAM. Carrasco KindNational Center for Supercomputing ApplicationsJ. CarreteroBarcelona Institute of Science and TechnologyF. J. CastanderInstitut d’Estudis Espacials de Catalunya (IEEC)R. CawthonWilliam Jewell CollegeC. L. ChangArgonne National LaboratoryC. ChangUniversity of ChicagoP. ChaubalUniversity of MelbourneR ChenDuke University DurhamH. C. ChiangMcGill UniversityA. ChoiNASA Goddard Space Flight CenterT.-L. ChouUniversity of ChicagoR. CitronUniversity of ChicagoC. Corbett MoranCalifornia Institute of TechnologyJ. CorderoUniversity of ManchesterM. CostanziINAF-Osservatorio Astronomico di TriesteT. M. CrawfordUniversity of ChicagoA. T. CritesCornell UniversityL. N. da CostaLaboratório Interinstitucional de e-Astronomia—LIneAM. E. S. PereiraUniversität HamburgC. DavisStanford UniversityT. M. DavisUniversity of QueenslandJ. DeRoseLawrence Berkeley National LaboratoryS. DesaiIIT HyderabadT. de HaanHigh Energy Accelerator Research Organization (KEK)H. T. DiehlFermi National Accelerator LaboratoryM. DobbsCanadian Institute for Advanced ResearchScott DodelsonCarnegie Mellon UniversityC. DouxUniversité Grenoble AlpesA. Drlica-WagnerFermi National Accelerator LaboratoryK. EckertUniversity of PennsylvaniaJ. Elvin-PooleUniversity of WaterlooS. EverettCalifornia Institute of TechnologyW. EverettUniversity of ColoradoI. FerreroInstitute of Theoretical AstrophysicsA. FertéSLAC National Accelerator LaboratoryA. M. FloresStanford UniversityJ. FriemanFermi National Accelerator LaboratoryJason GallicchioUniversity of ChicagoJ. García-BellidoUniversidad Autonoma de MadridM. GattiUniversity of PennsylvaniaE. M. GeorgeG. GianniniUniversity of ChicagoMichael D. GladdersUniversity of ChicagoD. GruenLudwig-Maximilians-UniversitätR. A. GruendlNational Center for Supercomputing ApplicationsN. GuptaAstronomy and SpaceG. GutierrezFermi National Accelerator LaboratoryN. W. HalversonUniversity of ColoradoI. HarrisonCardiff UniversityW. G. HartleyUniversity of GenevaK. HernerFermi National Accelerator LaboratoryS. R. HintonUniversity of QueenslandG. P. HolderUniversity of Illinois Urbana-ChampaignD. L. HollowoodSanta Cruz Institute for Particle PhysicsW. L. HolzapfelUniversity of CaliforniaK. HonscheidThe Ohio State UniversityJ. D. HrubesUniversity of ChicagoN. HuangUniversity of CaliforniaJohannes HubmayrNIST Quantum Devices GroupEric HuffCalifornia Institute of TechnologyDragan HutererUniversity of MichiganK. D. IrwinSLAC National Accelerator LaboratoryD. J. JamesCenter for Astrophysics | Harvard & SmithsonianMike JarvisUniversity of Pennsylvania
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Annotatsiya
In these two papers, the authors use mock maps to establish a method for studying the abundance and calibrating the weak-lensing based mass of galaxy clusters. They set up a likelihood function, thus obtaining cosmological constraints from a sample of 1,005 clusters detected with the South Pole Telescope, in combination with further cluster data from the Dark Energy Survey, the Wide-field Infrared Survey Explorer, and the Hubble Space Telescope.
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