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Fig. 3.

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Chandra X-ray images of the Spiderweb Galaxy field. Upper panels: Chandra ACIS-S images in the soft 0.5–2 keV (left) and hard 2–7 keV band (right). A box of 12 × 9 arcmin by side centered on J1140-2629 is shown. The images have been smoothed with a ∼1 arcsec Gaussian kernel to emphasize the unresolved sources. Sources at the outskirts of the image appear larger due to the effect of the increase of the PSF. Lower panels: close-up of the Spiderweb Galaxy (3 × 2 arcmin by side) at full angular resolution, in the soft (0.5–2 keV, left) and hard (2–7 keV, right) band. Extended emission is clearly visible in both bands. Red contours show radio emission observed in the 10 GHz band with the JVLA (see Carilli & Anderson 2022) at levels of 0.03, 0.2, 2 and 20 mJy beam−1.

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