Fig. 5.

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Best-fit spectrophotometric SED and Lyα model of the JWST data. The black solid curve shows the JWST/NIRSpec Prism spectrum and the dark blue dots the corresponding JWST/NIRCam photometry. The best-fit SED model from BAGPIPES is shown as the orange curve, here modified to include the DLA, with zabs as a free parameter. The best-fit MCMC stellar continuum and Lyα model is shown as the red dashed line, with a best-fit Lyα emission line redshift consistent with zspec but zabs = 5.396 ± 0.098.
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