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Fig. 5.

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PSF for HARMONI in the instrument configuration summaries in Table 3 at three wavelengths ranges. Upper panels: filter-band images (0.89−0.92 μm (left), 1.26−1.31 μm (centre), and 1.67−1.73 μm (right)). The 20 × 20 mas2 scale of our mock HARMONI observations undersamples the potential FWHM of the PSF, which varies from ∼6 mas at the bluest filter to ∼11 mas at the reddest one. Intensities are in logarithmic scale and normalised to the peak in each case. Lower panels: radial profiles along the right ascension axis and through the centre obtained from the filter-band image of the lenticular host galaxy scaled to 1011Lv, ⊙ without QSO (black profile), the QSO of L[OIII] = 1042 (red dashed-profile), and the QSO of L[OIII] = 1043 (blue dotted-line). Intensities are normalised to the peak of the host in each case.

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