[O III]88 μm spectrum (left) and flux map (right) of JADES-GS-z14-0. The top panel illustrates the redshift probability distribution determined from the JWST/NIRSpec data. The red vertical dotted line shows the redshift determined from the candidate C III] detection (Carniani et al. 2024). The black contours in the flux map show ±3, ±4, ±5, and ±6 σ of [O III]emission, while red contours correspond to the rest-frame UV emission from JWST/NIRCam F200W observations.