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机译:银河系卫星与费米大面积望远镜组合分析的约束暗物质模型
W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94305, USA;
W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94305, USA;
Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA;
Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, California 95064, USA;
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy;
dark matter (stellar, interstellar, galactic, and cosmological); ggr; -ray; dwarf galaxies (elliptical, irregular, and spheroidal);
机译:来自银河系矮星系和晕圈的费米大面积望远镜伽马射线数据的独立于模型的分析,以约束暗物质场景
机译:费米大面积望远镜检测器对银河系球面类星系的观测及对暗物质模型的约束
机译:费米大面积望远镜检测器对银河系球面类星系的观测及对暗物质模型的约束
机译:普通卤素表面密度为银河系和andromeda侏儒卫星作为暗物寒冷的探头
机译:使用费米LAT搜索银河系的暗物质卫星。
机译:使用全球定位系统卫星上的原子钟搜索畴壁暗物质
机译:银河系卫星与费米大面积望远镜组合分析的约束暗物质模型
机译:从银河卫星与费米大区域望远镜的组合分析约束暗物质模型。