Fig. 10
Distributions of limiting magnitude in the 3 HUGS images, as described in the legend. The lower x-axis shows the limiting magnitude computed at 1σ in an area of 1 arcsec2, the upper at 5σ in an area of 0.4 arcsec2, comparable to the average FWHM. Note that the latter is not the total magnitude of objects detected at 5σ in an area of 0.4 arcsec2, since no aperture correction has been applied.
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