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Fig. B.2.

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NIRSpec integrated spectrum of SW cone, showing the redshifted outflow. The black curve identifies the integrated spectrum, integrated over a circular region identified by the light-red crescent moon in the inset in Fig. 10; the total, multi-component best fit curve is in red, while the green and and grey Gaussian components show the systemic and outflow, respectively. The fit residuals are reported in the top panels. The most prominent emission lines are marked with grey vertical lines.

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