Plate 1 (file plate1.ps): 3.6 $\mu$m full frame PSF-roll subtracted image of Fomalhaut. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The ellipse indicates the location of the debris ring, and the cross the position of Fomalhaut b.

Plate 2 (file plate2.ps): 4.5 $\mu$m full frame PSF-roll subtracted image of Fomalhaut. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The ellipse indicates the location of the debris ring, and the cross the position of Fomalhaut b.

Plate 3 (file plate3.ps): 5.8 $\mu$m full frame PSF-roll subtracted image of Fomalhaut. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The ellipse indicates the location of the debris ring, and the cross the position of Fomalhaut b.

Plate 4 (file plate4.ps): 8.0 $\mu$m full frame PSF-roll subtracted image of Fomalhaut. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The ellipse indicates the location of the debris ring, and the cross the position of Fomalhaut b.

Plate 5 (file plate5.ps): 3.6 $\mu$m full frame PSF-roll subtracted image of $\epsilon$ Eridani. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The dotted circle indicates the position of the 20 AU asteroid belt, while the two dashed circles indicate the inner and outer boundaries of the sub-millimeter ring as derived by Backman et al. (2009).

Plate 6 (file plate6.ps): 4.5 $\mu$m full frame PSF-roll subtracted image of $\epsilon$ Eridani. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The dotted circle indicates the position of the 20 AU asteroid belt, while the two dashed circles indicate the inner and outer boundaries of the sub-millimeter ring as derived by Backman et al. (2009).

Plate 7 (file plate7.ps): 5.8 $\mu$m full frame PSF-roll subtracted image of $\epsilon$ Eridani. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The dotted circle indicates the position of the 20 AU asteroid belt, while the two dashed circles indicate the inner and outer boundaries of the sub-millimeter ring as derived by Backman et al. (2009).

Plate 8 (file plate8.ps): 8.0 $\mu$m full frame PSF-roll subtracted image of $\epsilon$ Eridani. The image is scaled linearly from 0 to 0.5 MJy/sr in surface brightness color scale. N is up and E is left. The dotted circle indicates the position of the 20 AU asteroid belt, while the two dashed circles indicate the inner and outer boundaries of the sub-millimeter ring as derived by Backman et al. (2009).