Made available in DSpace on 2022-04-29T08:39:05Z (GMT). No. of bitstreams: 0 Previous issue date: 2022-01-15; This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023514], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude...
Made available in DSpace on 2022-04-29T08:39:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2022-01-15; We present the first cosmology results from large-scale structure using the full 5000 deg2 of imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis of large-scale structure combining three two-point correlation functions (3×2pt): (i) cosmic shear using 100 million source ...
Made available in DSpace on 2022-04-29T08:28:07Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-06-07; We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, ΛCDM and wCDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data....
Made available in DSpace on 2022-04-29T08:29:09Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-01-21; We analyze Dark Energy Survey (DES) data to constrain a cosmological model where a subset of parameters - focusing on ωm - are split into versions associated with structure growth (e.g., ωmgrow) and expansion history (e.g., ωmgeo). Once the parameters have been specified for the ΛCDM cosmological model,...
Made available in DSpace on 2022-04-29T08:29:42Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-06-15; We study a phenomenological class of models where dark matter converts to dark radiation in the low redshift epoch. This class of models, dubbed DMDR, characterizes the evolution of comoving dark-matter density with two extra parameters, and may be able to help alleviate the observed discrepancies betwe...
Made available in DSpace on 2021-06-25T10:51:09Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-01-01; Natural Sciences and Engineering Research Council of Canada; Fakulta Elektrotechniky a Informatiky, Vysoká Škola Bánská - Technická Univerzita Ostrava; Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica; Corporación de Fomento de la Producción; Seventh Framework Programme; ...
Made available in DSpace on 2021-06-25T12:34:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-01-21; Porat Fellowship at Stanford University; Rackham Graduate School; National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility; Stanford University; Stanford Research Computing Center; U.S. Department of Energy; U.S. National Science Foundatio...
Made available in DSpace on 2019-10-06T16:24:15Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-09-01; Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica; Seventh Framework Programme; Horizon 2020; Consejo Nacional de Innovación, Ciencia y Tecnología; Ministerstvo Školství, Mládeže a Tělovýchovy; Uddannelses- og Forskningsministeriet; Ministerio de Economía, Industria y Comp...
Made available in DSpace on 2019-10-04T12:38:36Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-06-07; U.S. Department of Energy; U.S. National Science Foundation; Ministry of Science and Education of Spain; Science and Technology Facilities Council of the United Kingdom; Higher Education Funding Council for England; National Center for Supercomputing Applications at the University of Illinois at Urbana-...
e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV - the lower energy limit can be pushed to energies as low as 150 keV for the tracker, and to 30 keV for calorimetric detection. The mission is ba...