SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets
S. BocquetLudwig-Maximilians-UniversitätS. GrandisLudwig-Maximilians-UniversitätL. E. BleemArgonne National LaboratoryMatthias KleinLudwig-Maximilians-UniversitätJ. J. MohrLudwig-Maximilians-UniversitätM. AguenaLaboratório Interinstitucional de e-Astronomia - LIneAA. AlarconArgonne National LaboratoryS. AllamFermi National Accelerator LaboratoryS. W. AllenSLAC National Accelerator LaboratoryO. AlvesUniversity of MichiganA. AmonUniversity of CambridgeBehzad AnsarinejadUniversity of MelbourneDavid BaconUniversity of PortsmouthM. BaylissUniversity of CincinnatiK. BechtolUniversity of Wisconsin-MadisonM. R. BeckerArgonne National LaboratoryB. A. BensonFermi National Accelerator LaboratoryG. M. BernsteinUniversity of PennsylvaniaM. BrodwinUniversity of MissouriDavid BrooksUniversity College LondonA. CamposCarnegie Mellon UniversityRebecca CanningUniversity of PortsmouthJ. E. CarlstromArgonne National LaboratoryA. Carnero RosellInstituto de Astrofisica de CanariasM. Carrasco KindUniversity of Illinois at Urbana-ChampaignJ. CarreteroBarcelona Institute of Science and TechnologyR. CawthonWilliam Jewell CollegeC. ChangUniversity of ChicagoR ChenDuke University DurhamA. ChoiNASA Goddard Space Flight CenterJ. CorderoUniversity of ManchesterM. CostanziINAF-Osservatorio Astronomico di TriesteL. N. da CostaLaboratório Interinstitucional de e-Astronomia - LIneAM. E. S. PereiraUniversität HamburgC. DavisStanford UniversityJ. DeRoseLawrence Berkeley National LaboratoryS. DesaiIIT HyderabadT. de HaanHigh Energy Accelerator Research Organization (KEK)J. De VicenteCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT)H. T. DiehlFermi National Accelerator LaboratoryScott DodelsonCarnegie Mellon UniversityP. DoelUniversity College LondonC. DouxUniversity of PennsylvaniaA. Drlica-WagnerFermi National Accelerator LaboratoryK. EckertUniversity of PennsylvaniaJ. Elvin-PooleUniversity of WaterlooS. EverettCalifornia Institute of TechnologyI. FerreroInstitute of Theoretical AstrophysicsA. FertéSLAC National Accelerator LaboratoryA. M. FloresStanford UniversityJoshua A. FriemanFermi National Accelerator LaboratoryJ. García-BellidoUniversidad Autonoma de MadridM. GattiUniversity of PennsylvaniaG. GianniniBarcelona Institute of Science and TechnologyMichael D. GladdersUniversity of ChicagoD. GruenLudwig-Maximilians-UniversitätR. A. GruendlCenter for Astrophysical SurveysI. HarrisonCardiff UniversityW. G. HartleyUniversity of GenevaK. HernerFermi National Accelerator LaboratoryS. R. HintonUniversity of QueenslandD. L. HollowoodSanta Cruz Institute for Particle PhysicsW. L. HolzapfelUniversity of CaliforniaK. HonscheidThe Ohio State UniversityN. HuangUniversity of CaliforniaE. M. HuffCalifornia Institute of TechnologyD. J. JamesCenter for Astrophysics | Harvard & SmithsonianMike JarvisUniversity of PennsylvaniaGourav KhullarUniversity of ChicagoKeunho KimUniversity of CincinnatiRobert P. KraftCenter for Astrophysics | Harvard & Smithsonian, CambridgeK. KuehnLowell ObservatoryN.P. KuropatkinFermi National Accelerator LaboratoryF. KéruzoréArgonne National LaboratoryS. LeeCalifornia Institute of TechnologyP.-F. LégetStanford UniversityN. MacCrannUniversity of CambridgeGuillaume MahlerDurham UniversityA. MantzStanford UniversityJ. L. MarshallTexas A&M UniversityJ. McCulloughStanford UniversityM. McDonaldMassachusetts Institute of TechnologyJ. Mena-FernándezCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT)R. MiquelBarcelona Institute of Science and TechnologyJ. MylesSLAC National Accelerator LaboratoryA Navarro-AlsinaUniversidade Estadual de CampinasR. L. C. OgandoA. PalmeseCarnegie Mellon UniversityS PandeyUniversity of PennsylvaniaA. PieresLaboratório Interinstitucional de e-Astronomia - LIneAA. A. Plazas MalagónSLAC National Accelerator LaboratoryJ. PratUniversity of ChicagoM. RaveriUniversity of Genova and INFNC. L. ReichardtUniversity of MelbourneJoseph RobersonUniversity of CincinnatiR. P. RollinsUniversity of ManchesterA. K. RomerUniversity of SussexC. RomeroCenter for Astrophysics | Harvard & SmithsonianA. RoodmanSLAC National Accelerator LaboratoryA.J. RossThe Ohio State University
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Аннотация
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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