Only the star was detected at 24$\mu$m ($270.3 \pm 0.1$mJy), but this observation provides confirmation of the 99 Her stellar position in the PACS images relative to a background object 1.8 arcmin away to the SE ($PA=120^\circ$) that is visible at 24, 70, and 100$\mu$m. The presence of an excess at 70$\mu$m ($98 \pm 5$mJy compared to the photospheric value of 30mJy) was in fact reported by @2010ApJ...710L..26K. They did not note either the circumbinary nature or that the disk may be marginally resolved by MIPS at 70$\mu$m. Because our study focuses on the spatial structure, we use the higher resolution PACS data at 70$\mu$m, but include the MIPS data to model the SED.

Basic image analysis {#s:basic}
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Figure \[fig:pacs\] shows the *Herschel* PACS data. Compared to the beam size, the disk is clearly resolved at all three wavelengths. At 160$\mu$m the peak is offset about 5” East relative to both the 70 and 100$\mu$m images. However, the disk is still visible at 160$\mu$m as the lower contours match the 70 and 100$\mu$m images well. The 160$\mu$m peak is only 2-3$\sigma$ more significant than these contours. While such variations are possible due to noise, in this case the offset 