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Fig. 4.

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Source-integrated spectrum of 3C 326 N from the NIRSpec observation from 1.5 to 2.9 μm showing most of the lines. The flux was extracted with an elliptical aperture centred on the peak continuum flux with a major axis along Dec of 1.1″ and a minor axis of 0.9″. Empty pixels were not included and the pixels within the aperture were sigma clipped with a tolerance of 5σ. The spectral gap at 2.2 μm is caused by the NIRSpec IFU detector gap.

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