Extended Data Fig. 1: X-ray structures within the Perseus core and default radial binning scheme adopted for the analysis. | Nature

Extended Data Fig. 1: X-ray structures within the Perseus core and default radial binning scheme adopted for the analysis.

From: Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

Extended Data Fig. 1

(a) Residual X-ray/Chandra image of the Perseus cluster in the 2−8 keV band, with arrows highlighting prominent structures relevant to our analysis. (b) The color pixels and grey circles/annuli show detector and sky regions (No. 1–6 from inner to outer), respectively, with the black dashed circle marking the innermost sky region. White contours illustrate the regions that contribute 90% photons to each pointing based on our SIXTE simulations.

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