of the rest of this paper is as follows. Section 2 describes the sample selection and the observations; Sections 3 and 4 present the results of the survey, in the form of a table, spectra, and comments on individual objects; and Section 5 gives gives a brief discussion. A detailed analysis of the results will given in a separate paper.

The Survey
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Survey Sample
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The survey PNe were taken from the Strasbourg-ESO Catalog of Galactic PNe (Acker et al. 1992) and were chosen to include a major component of relatively young PNe with a broad range of spectroscopic characteristics. The PNe were selected to have small angular diameters ($\la$ the telescope beam size whose FWHM is $12\arcsec$), relatively high fluxes in H$\alpha$ (with a few exceptions $>10^{-13}$ erg cm$^{-2}$ s$^{-1}$, uncorrected for reddening), and consequently moderate to high surface brightness in the Balmer lines and the radio continuum. The PNe lie close to the galactic plane, and the practical declination limit set by the telescope location is $\sim
-$25. In addition, the PNe were distributed among different spectroscopic groups, based on line ratios given in the PN catalog, or updated from the literature: 1) \[O[iii]{}\] $\lambda$5007/H$\beta <
6.0$ 