Fig. A.4.
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Ratio of the flux measured from the Sérsic model of The Cliff to the observed NIRCam image within the rectangular aperture of the NIRSpec microshutter. Error bars reflect both the uncertainty in the Sérsic fitting and the exact pointing location of JWST. Emission from The Cliff dominates (> 80%) the total observed flux at all wavelengths, and accounts for ∼100% of the total emission redward of the Balmer break (> 2μm).
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