Fig. 3.

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Fourier analysis for NGC 3772, taken as an example. From top to bottom: non-deprojected SDSS r-band image of the galaxy, radial profiles of the relative amplitude of the m = 1, 2, 3, and 4 Fourier components, radial profiles of the bar/interbar intensity ratio used to derive the bar radius, marked by the vertical dashed line.
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