The Classifications and Some Correlations for Fermi Blazars
Center for Astrophysics, Guangzhou University, Guangzhou 510006, China
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province, Guangzhou 510006, China
Department of Physics and Electronics Science, Hunan University of Arts and Science, Changde 415000, China
Author to whom correspondence should be addressed.
Academic Editors: Jose L. Gómez, Alan P. Marscher and Svetlana G. Jorstad
Received: 14 July 2016 / Revised: 17 August 2016 / Accepted: 17 August 2016 / Published: 29 August 2016
PDF [1430 KB, uploaded 29 August 2016]
In a recent paper, we constructed the spectral energy distributions (SEDs) for 1425 Fermi blazars. We classify them as low synchrotron peak sources (LSPs) if log
14.0, intermediate synchrotron peak sources (ISPs) if
, and high synchrotron peak sources (HSPs) if
. We obtain an empirical relation to estimate the synchrotron peak frequency,
from effective spectral indexes
. In the present work, we investigate the correlation between the peak frequency and the radio-to-X-ray spectral index, between peak luminosity (bolometric luminosity) and γ
-ray/optical luminosity, and between peak luminosity and bolometric luminosity. Some discussion is presented.
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MDPI and ACS Style
Fan, J.; Liu, Y.; Yang, J.; Lin, C.; Hao, J.; Xiao, H. The Classifications and Some Correlations for Fermi Blazars. Galaxies 2016, 4, 16.
Fan J, Liu Y, Yang J, Lin C, Hao J, Xiao H. The Classifications and Some Correlations for Fermi Blazars. Galaxies. 2016; 4(3):16.
Fan, Junhui; Liu, Yi; Yang, Jianghe; Lin, Chao; Hao, Jingmeng; Xiao, Hubing. 2016. "The Classifications and Some Correlations for Fermi Blazars." Galaxies 4, no. 3: 16.
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