2017
DOI: 10.1007/s10509-016-3002-y
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The γ $\gamma$ -ray spectral changes in Fermi blazars

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Cited by 8 publications
(2 citation statements)
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“…Through the log-parabolic model fitting, 12 fitting parameters can be obtained as β syn , β ic , log ν syn peak , log ν ic peak , log L syn peak , log L ic peak , and the spectral index α ν of each band: the radio (1.4 GHz), infrared (2.2 µm), optical (J band, 1250 nm), ultraviolet (250 nm), soft X-ray (1 keV) and γ-ray (20 GeV) bands (Fossati et al 1998;Nie et al 2014;Yang et al 2017). We can also calculate the physical parameters indirectly, including D, R, B and γ p .…”
Section: The Intrinsic Physical Parametersmentioning
confidence: 99%
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“…Through the log-parabolic model fitting, 12 fitting parameters can be obtained as β syn , β ic , log ν syn peak , log ν ic peak , log L syn peak , log L ic peak , and the spectral index α ν of each band: the radio (1.4 GHz), infrared (2.2 µm), optical (J band, 1250 nm), ultraviolet (250 nm), soft X-ray (1 keV) and γ-ray (20 GeV) bands (Fossati et al 1998;Nie et al 2014;Yang et al 2017). We can also calculate the physical parameters indirectly, including D, R, B and γ p .…”
Section: The Intrinsic Physical Parametersmentioning
confidence: 99%
“…We can also calculate the physical parameters indirectly, including D, R, B and γ p . In addition, we can calculate the γ-ray luminosity at E = 20 GeV by the following formula (Fan et al 2012(Fan et al , 2015Nie et al 2014;Yang et al 2017):…”
Section: The Intrinsic Physical Parametersmentioning
confidence: 99%