Examples of our multicomponent decompositions. Large panel: black dots show the surface brightnesses (r′ magnitude/arcsec²) of the pixels in the two-dimensional image, white dots the values in the final model image, and the colors the values corresponding to the different structure components of the model. Bulges, disks, and barlenses were fitted with a Sérsic function, and bars with a Ferrers function. The decomposition parameters, galaxy masses (log M_⋆), galaxy inclinations (i), and Hubble stages (T) are shown in the upper right. Lower panels (from left to right): region of the r′-band SDSS mosaic image, the same image with the model components plotted on top of that, and the unsharp mask image. The image in the large panel shows the full galaxy image. For more examples, see Appendix E.