Fig. 1.
Smoothed flux image of Abell 3411 combined from 1.2–4.0 keV XMM-Newton EPIC CCDs (left), 0.7–7.0 keV Suzaku XIS CCDs (middle), and 1.2–4.0 keV Chandra ACIS-I (right). Particle background and vignetting effect have been corrected. White contours are GMRT 610 MHz radio intensity. XMM-Newton and Suzaku analysis regions are plotted with cyan sectors. The locations of two BCGs are plotted with red crosses in the Chandra image. The coordinates of the BCGs are obtained from Golovich et al. (2019a).
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