Fig. C.1.
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Comparison between radial profiles derived using a 1.2 kpc slit through the semi-major axis of the galaxy (solid, cyan) and elliptical annuli (dashed, black) for UGC09138 (edge-on, top panels) and NGC1042 (low-inclination, lower panels). The elliptical annuli method is suitable for the low-inclination galaxies studied in this work. See text for details.
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