3.6 μm photometry for NGC 891. Top panel: distribution of light in the sky in thin (blue) contours overlaid with our best model with bulge and thin and thick disks, see Table 4. Bottom left: light distribution along the vertical direction above and below the plane (circles and triangles) compared with our best model (thick blue curve). Bottom right: light distribution along the plane of the galaxy (circles and triangles) compared with our best model (thick blue curve).
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