new RP catalog objects, and to use any detections to illuminate a) the veracity of the PN designations, particularly for cases were the classifications in the RP catalog were uncertain, b) the nebular dimensions and morphological features, c) the location and characteristics of the central stars, and d) strategies for follow-up observations of the RP sample. In §2, we describe the RP catalog of LMC PNe and the survey upon which it is based, and then describe the observational data extracted from the [*HST*]{} archive that matches the new sources in the RP catalog. The individual objects are described in §3, along with an analysis of non-detections. In §4 we discuss the implications of these data for future observing programs.

Observational Data
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The surveys upon which the RP catalog of LMC PNe is based, the observing strategies, the discovery technique, the follow-on spectroscopy, and the classification schema are all described by [@RP06a; @RP06b]. We summarize in the next subsection some of the key features of the RP survey and discovery images in enough detail to explain the comparison to the serendipitous [*HST*]{} images. Following that we describe the attributes of the [*HST*]{} observations, the reduction procedures, and our analysis 