summarize the observational details for our sample. The apertures from which our fluxes were extracted are listed in Table 2 and correspond to either the size of a single slit if the galaxy was observed as a staring observation, or the maximum overlap aperture between the SH and LH maps such that both the SH and LH spectra correspond to the same physical region on the sky. For the [*SINGS*]{} observations, this corresponds to roughly a 23”$\times$15” aperture. In some mapping observations, the \[NeV\] line was detected in a small aperture, but not in the largest possible extraction region. In these cases, the aperture used to obtain the \[NeV\] detection is listed in Table 2. Here, identical apertures for both the SH and LH modules were also used so that spectra from both modules corresponded to the same physical region.

[lclccrlcc]{}\
\
& & & Exposure & Exposure & & Extraction &\
& & & Time SH & Time LH & & & Aperture &\
& & & & & & & Size SH &\
& & & (4) & (5) & & & (8) &\
\
\
NGC925 & 159 & Mapping & 60 & 60 & 02:27:16.90 & 