Fig. 2.
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NIRSpec spectra obtained with internal (orange curve) and external (green) flux calibration and integrated over a region of r = 1.5″. The two NIRSpec spectra are extracted from the drizzle cubes, with 0.05″ spaxels. Vertical lines indicate the main emission line features detected in the NIRSpec spectrum. The inset shows the same NIRSpec spectra compared with the Magellan/FIRE (magenta) and the SDSS (purple) spectra, rescaled by a factor of 1.6 to match the NIRSpec spectra in the vicinity of the Hβ and [O III] lines.
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