it is also possible to extract spectral images over a certain wavelength range (e.g., over a particular line or a continuum) to recover the spatial extent of a specific emission. Fig.\[6781example\] shows footprints of detector apertures for , the target PN we consider in detail in this paper, to illustrate how each of these data sets was obtained. In the forthcoming papers of the HerPlaNS series, we will discuss the broadband mapping and spectroscopic data separately for the entire HerPlaNS sample of 11 PNs plus others in the archive.

[lcccccccc]{}

\
Object & OD & Pointing & RA (2000) & DEC (2000) & AOT & Duration & Start Date & Time & Obs. Id\
& & & (h m s) & (d m s) & & (Sec) & (UTC) &\

\
Object & OD & Pointing & RA (2000) & DEC (2000) & AOT & Duration & Start Date & Time & Obs. Id\
& & & (h m s) & (d m s) & & (Sec) & (UTC) &\
NGC40 & 788 & Center & 00 13 01.010 & $+$72 31 19.10 & PacsPhoto & 15038 & 2011-07-10T18:34:30Z & 1342223905\
& 788 & Center & 00 13 01.010 & 