Fig. 14.

Top row panels: comparison of the input structural parameters of the mock galaxies to the values measured by our photometric pipeline. The shown parameters are apparent magnitude (mr′), effective radius in arcsec (Re), position angle (θ), axis ratio (b/a), and Sérsic index (n), and the blue diagonal lines represent the 1:1 ratio. Second and third row panels: mean differences between the input and output parameters (input – output) as a function of their input and output mean effective r′-band surface brightness, , respectively. Bottom row: standard deviations of the input – output parameter differences as a function of the input mean
. The dotted lines in the bottom row panels show the fits to the standard deviations as defined in Eq. (10).
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