Fig. 11.
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Historical 2–10 keV light curve of IC 4329A as observed with various X-ray satellites. In chronological order: Einstein, 1979 (Holt et al. 1989); EXOSAT, 1985 (Singh et al. 1991); Ginga, 1989 (Piro et al. 1990); BeppoSAX, 1998 (Dadina 2007); Chandra, 2001 (Shu et al. 2010); XMM-Newton 2001, 2003 (Nandra et al. 2007); Suzaku, 2007 (Mantovani et al. 2014); Swift/XRT, 2007 (Winter et al. 2009); AstroSat, 2017 (Tripathi et al. 2021); XMM-Newton 2022; medium flux of the observations analyzed in this work.
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