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- W3100291466 endingPage "120" @default.
- W3100291466 startingPage "120" @default.
- W3100291466 abstract "In this work, we collected a sample of 69 TeV blazars from TeVCat, obtained their multi-wavelength observations, and fitted their spectral energy distributions by using the second degree polynomial function. The structure parameters of the synchrotron bumps for 68 blazars and those of the inverse-Compton bumps for 56 blzars are obtained. Then, we adopted statistical analysis to the parameters (curvature, peak frequency, peak luminosity, bolometric luminosity, and X/$gamma$-ray spectral indexes). From our analysis and discussions, we can get following conclusions: 1. There is a clear positive correlation between the synchrotron peak frequency, $log nu_p^s$, and the inverse-Compton peak frequency $log nu_p^{IC}$, and that between the synchrotron peak luminosity, $log nu_p^s L_p^s$, and the inverse-Compton peak luminosity, $log nu_p^{IC}L_p^{IC}$. 2. The correlation between the peak frequency and the curvature of synchrotron bump is clearly different from that of the inverse-Compton bump, which further indicates that there are different emission mechanisms between them. 3. There is a correlation between $log nu_p^{IC}$ and $gamma$-ray spectral index, $alpha_gamma$, for the TeV blazars: $log nu^{IC}_p = -(4.59 pm 0.30) alpha_gamma + (32.67 pm 0.59)$, which is consistent with previous work of Abdo et al.(2010). 4. An L-shape relation is found between $log nu^s_p$ and $alpha_X$ for both TeV blazars and Fermi blazars. A significant correlation between $log nu^s_p$ and X-ray photon index ($alpha_X$) is found for the TeV blazars with high synchrotron peak frequency: $log nu^{s}_{p} = -(3.20 pm 0.34) alpha_X + (24.33 pm 0.79)$, while the correlation is positive for low synchrotron peaked TeV sources. 5. In the $alpha_X-alpha_gamma$ diagram, there is also an L-shape, the anti-correlation is consistent with the available results in the literature, (...)" @default.
- W3100291466 created "2020-11-23" @default.
- W3100291466 creator A5014885678 @default.
- W3100291466 creator A5081922643 @default.
- W3100291466 date "2018-10-01" @default.
- W3100291466 modified "2023-10-16" @default.
- W3100291466 title "Spectral energy distributions for TeV blazars" @default.
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- W3100291466 doi "https://doi.org/10.1088/1674-4527/18/10/120" @default.
- W3100291466 hasPublicationYear "2018" @default.
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