Fig. 5.
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Examples of photometric decomposition for galaxies in the edge-on view (ID = 513105, 455292). The first column shows the edge-on mock image generated using the GALAXEV pipeline. The dashed red line, located 1Re from the galaxy center, divides the edge-on galaxy into part 1 and part 2. The second column presents the three-component (bulge+disk+stellar halo) model fit by GALFIT. The third column displays the residual of this fitting result. The fourth column shows the one-dimensional surface brightness of different components along the major axis that is oriented to be aligned with the x axis.
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