Fig. 3
Pseudo-color RGB image of the Coma cluster field based on a combination of 0.3–0.6, 0.6–1.0, and 1.0–2.3 keV images. The diffuse emission, which is dominated by the Milky Way contribution appears red in this image. Distant AGNs and a few galactic sources (including stars) span full range of colors. Clusters of galaxies, including the Coma cluster itself, appear as extended white objects in this image.
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