Visual Method for Spectral Energy Distribution Calculation of Blazars

被引:0
作者
Y. Huang
J. H. Fan
机构
[1] Guangzhou University,School of Computer Science and Education Software
[2] Guangzhou University,Centre for Astrophysics
[3] Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province,undefined
来源
Journal of Astrophysics and Astronomy | 2014年 / 35卷
关键词
Galaxies: active; galaxies: BL Lacertae objects; galaxies: quasars; galaxies: emission;
D O I
暂无
中图分类号
学科分类号
摘要
In this work, we propose to use ‘The Geometer’s Sketchpad’ to the fitting of a spectral energy distribution of blazar based on three effective spectral indices, αRO, αOX, and αRX and the flux density in the radio band. It can make us to see the fitting in detail with both the peak frequency and peak luminosity given immediately. We used our method to those sources whose peak frequency and peak luminosity are given and found that our results are consistent with those given in the work of Sambruna et al. (1996).
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页码:507 / 508
页数:1
相关论文
共 14 条
  • [1] Abdo AA(2010)undefined ApJS 188 405-undefined
  • [2] Ackermann M(2013)undefined RAA 13 259-undefined
  • [3] Ajello M(1998)undefined MNRAS 299 433-undefined
  • [4] Fan JH(1986)undefined ApJ 308 78-undefined
  • [5] Yang JH(1996)undefined ApJ 463 444-undefined
  • [6] Liu Y(undefined)undefined undefined undefined undefined-undefined
  • [7] Zhang JY(undefined)undefined undefined undefined undefined-undefined
  • [8] Fossati G(undefined)undefined undefined undefined undefined-undefined
  • [9] Maraschi L(undefined)undefined undefined undefined undefined-undefined
  • [10] Celotti A(undefined)undefined undefined undefined undefined-undefined