Fig. 4
Examples of simulated images of galaxies with random ellipticities. Signal-to-noise ratios from left to right and top to bottom: ν = 10, 20, 40, and 200. The radial light profile of the pre-seeing images is exponential with rh = 0.2′′; the pixel size is 0.1′′. The FWHM of the PSF is indicated by the circle in the top right corners.
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