Image Details
Caption: Figure 3.
The ALMA sources in the UNCOVER region (open squares using the color notation of Figure 2) overlaid on the 0.5–7 keV Chandra image. In the top panel, we show the X-ray image, which emphasizes the impact of the cluster foreground emission. In the bottom panel, we have subtracted a ﹩7\mathop{.}\limits^{^{\prime\prime} }5﹩ median-smoothed image to show the point sources in the region of the cluster atmosphere. The black contour shows the JWST UNCOVER area.
© 2026. The Author(s). Published by the American Astronomical Society.