5 years ago

Swift Observations of Mrk 421 in Selected Epochs. I. The Spectral and Flux Variability in 2005–2008

We present detailed results of Swift observations of the nearby TeV-detected blazar Mrk 421, based on the rich archival data obtained during 2005 March–2008 June. The best fits of the 0.3–10 keV spectra were mainly obtained using the log-parabolic model, yielding low spectral curvatures expected in the case of the efficient stochastic acceleration of particles. During strong X-ray flares, the position of the synchrotron spectral energy distribution peak ##IMG## [http://ej.iop.org/images/0004-637X/854/1/66/apjaaa75dieqn1.gif] {${E}_{{\rm{p}}}$} was beyond 8 keV for 41 spectra, while it sometimes was situated at the UV frequencies in quiescent states. The photon index at 1 keV exhibited a broad range, and the values ##IMG## [http://ej.iop.org/images/0004-637X/854/1/66/apjaaa75dieqn2.gif] {$a\lt 1.70$} were observed during the strong flares, hinting at the possible presence of a jet hadronic component. The spectral parameters were ...

Publisher URL: http://iopscience.iop.org/0004-637X/854/1/66

DOI: 10.3847/1538-4357/aaa75d

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