Long-term X-ray and TeV gamma-ray fluxes are linearly correlated in most HBL blazars, with steeper indices for Mrk 501 and the 2006 PKS 2155-304 flare.
Multi-wavelength Observations of Markarian 501
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abstract
The very high energy (VHE; E > 100 GeV) gamma-ray blazar Markarian 501 has a history of extreme spectral variability and is an excellent laboratory for studying the physical processes within the jets of active galactic nuclei. A short term multi-wavelength study of Markarian 501 was coordinated in March 2009 using the Suzaku X-ray satellite as well as the VERITAS and MAGIC experiments to cover the critical X-ray and VHE gamma-ray bands. The results of the quiescent-state observations with VERITAS and Suzaku are combined with public data from the Fermi Gamma-ray Space Telescope and compared to historical observations of the source during an extreme outburst, to examine the spectral variability, particularly how the spectral energy distribution varies with flux.
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On the correlation between X-rays and TeV gamma-rays in HBL Blazars
Long-term X-ray and TeV gamma-ray fluxes are linearly correlated in most HBL blazars, with steeper indices for Mrk 501 and the 2006 PKS 2155-304 flare.