Fig. 8.
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Measurements of the MXDF LSF in the combined datacube (not sky subtracted). The bottom panel displays the fitted Gaussian FWHM for a few bright sky lines. Variations with the field of view are given by the error bars (standard deviation). The DR1 UDF-10 polynomial approximation is shown as a dashed line. Examples of FWHM spatial maps are given for three sky lines in the top panels. FWHM units is Å.
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