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The Relations of Multi-waveband Effective Spectral Indices for Fermi Blazars
Affiliation:1. College of Mathematics and Physics Science, Hunan University of Arts and Science, Changde 415000;2. Center for Astrophysics, Guangzhou University, Guangzhou 510006;1. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030;2. Beijing Satellite Navigation Center, Chinese Academy of Sciences, Beijing 100092;3. National Defenses University, Beijing 100091;1. Key Laboratory foe Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210033;2. University of Chinese Academy of Sciences, Beijing 100049;3. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026;1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023;2. Key Laboratory of Dark Matter and Space Astronomy, Chinese Academy of Sciences, Nanjing 210023;3. School of Computer Science and Technology, Wuhan University of Technology, Wuhan 430070;4. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026;5. State Key Laboratory for Novel Software Technology, Nanjing University, Nanjing 210023;1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023;2. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026;3. CAS Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023;1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210033;2. Key Laboratory of Planetary Sciences, Chinese Academy of Sciences, Nanjing 210033;3. School of Astronomy and Space Science, Nanjing University, Nanjing 210023
Abstract:
Keywords:Galaxy: active  Radiation mechanism: non-thermal  effective spectral index: multi-waveband  method: statistical
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