Left: Chandra image of M87 in the 3–7 keV energy band. The sky regions used for ray tracing and arf generation are overplotted in white. We neglect scattering from regions located beyond 5.2 arcmin from the center (shown as the outer white circle), hence the image is set to zero here. Right: Chandra image of M87 in the 0.5–2 keV energy band, divided by a spherically symmetric beta model to highlight substructure related to AGN feedback. In particular the bright E and SW arms can be easily seen. The four XRISM/Resolve fields of view used to map the core of M87 are shown in white. Both images correspond to the same sky coordinates.