Fig. 18.
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Four representative spectra of Mrk 3 in units of E * F(E) with the best-fit modeling for the LHS (ASCA observation with ID = 70002000 in panel a), IS (Suzaku observation with ID = 100040010 in panel b), IS (RXTE observation with ID = 20330-01-09-00 in panel c) and IS (BeppoSAX observation with ID = 50132002 in panel d) states. The data are denoted by crosses, while the spectral model is shown by a red histograms for each state. Bottom: Δχ vs photon energy in keV.
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