the South African Astronomical Observatory, the 2.3-m telescope at Siding Spring Observatory, and 6dF on the UKST. However, the vast majority were confirmed using 2dF on the Anglo Australian Telescope (AAT) in 2004 December [see @RP06b].

AAO 2dF Fiber Spectra
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Confirmatory spectra were obtained for nearly every object in the RP catalog [@Reid06]. All of the spectra for the objects presented here were obtained with the AAO 2dF spectrograph on the AAT, which is capable of obtaining more than 400 simultaneous spectra, using a 300 line mm$^{-1}$ grating to cover the spectral range 3650–8050ÅÅwith a dispersion of 4.3 Å pixel$^{-1}$. The spectra were corrected for detector bias, extracted, and sky-subtracted. The wavelength calibration was performed with the aid of comparison arcs taken during the course of the observations, but no flux calibration was performed. See @RP06b and @Reid06 for details of the reductions. The spectrograms are shown in Figures \[Spec\_1\] and \[Spec\_2\]; the flux scale is in instrumental units.

HST Images
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Our search of the [*HST*]{} archive (conducted in 2006 June) identified nearly 200 images that were coincident with 19 of the newly discovered PNe candidates in the RP catalog, or about 4.0% of the sample of new 