accuracy of the reductions is not critical. However we did combine images taken with the same filter, when possible, to eliminate cosmic rays and to improve the signal-to-noise ratio for presentation. The [*HST*]{} observing log for all nebulae is presented in Table \[ObsLog\]. The first column lists the RP designation, followed by the confidence with which @RP06b could establish the target as a genuine PN based on their imaging and confirmatory spectroscopy, followed by their estimate of the diameter of the nebular shell. This information is followed in the next two columns by the [*HST*]{} observing configuration, followed by the exposure time and whether extended emission was detected. The last column lists the dataset identifiers in the MAST archive, which corresponds to high-level science products (i.e., combined images as generated through, e.g., the WFPC2 Archival Pure Parallels Project pipeline) where available.

Dimensions and Morphology for the Matched Sources
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The [*HST*]{} and matching RP catalog images for the detected nebulae are presented in Figures \[Neb\_1\] through \[Neb\_4\], where for each object we show both the UKST discovery image and the [*HST*]{} image on the same spatial scale. All of the images are rendered in false-color, usually with a square-root intensity 