Fig. 13.

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JWST/NIRCam F115W/F200W/F444W cutout showing the close environment of GS133. The red dashed box marks the NIRSpec IFS FOV, while the white contours show the Chandra 0.5–7 keV emission from Luo et al. (2017), highlighting the position of two X-ray AGN with a projected separation of ∼130 kpc and a velocity offset of ∼5000 km s−1 (Δz = 0.08). The apparent offset between the NIR and X-ray positions can be attributed to Chandra’s low angular resolution and the fact that the Chandra image is composed of multiple observations taken with varying aim points and roll angles. The inset shows a zoom-in on GS133. The images are oriented north up, east left.
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