Fig. 4.
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Flux-density-to-counts ratio for the gratings (IzJ-blue and H + K-dashed red lines) used for the mock HARMONI observations of AGNs+hosts. We note that the derived functions only cover the Hβ+MgI spectral range (4770−5400 Å rest-frame wavelengths) at redshifts 0.76 (1), 1.50 (2), and 2.30 (3) due to the design of our simulations.
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