Quasar-subtracted [O III] λ5007 emission map from the NIRSpec IFU (grey image) compared to the [C II] 158 μm emission map (orange contours) and the rest-frame 158 μm FIR continuum emission map (purple contours) from ALMA (see Section 5.2). The [C II] 158 μm contours are linearly spaced from 5σ to 26σ, where σ = 16 μJy. The FIR continuum contours are linearly spaced from 5σ to 42σ, where σ = 7 μJy/beam. The grey circle depicts the approximate PSF of the ALMA observations, with beam diameter $0\stackrel{″}{.}3$. The green cross marks the peak of the quasar emission from the NIRSpec IFU data that has been astrometrically aligned to the NIRCam imaging, which is aligned to Gaia DR2 (Yue et al. 2024). The purple circle marks the peak of the 158 μm FIR continuum emission reported by Venemans et al. (2017). The blue diamond marks the original quasar position from UKIDSS quoted by Mortlock et al. (2011).