RP images owing to the response of the photographic media, as explained by @RP06b. Our assessment of whether the object is a genuine PN is given in column (5), and the nebular morphological classification is given in column (6). Column (7) contains specific notes about each object, including whether a central star was identified.

Detected Objects
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As discussed in the previous section, extended emission was detected in the [*HST*]{} archival images for eight RP catalog objects. We describe here the morphological details and noteworthy spectral features for each of the nebulae listed in Table \[Morph\].

[*LMC–RP 265.—*]{}The [*HST*]{} image for this object was presented by @Shaw_etal06. Although it is extremely faint, it is probably a bipolar. The spectrum in Figure \[Spec\_1\] indicates a moderate excitation, owing to the modest \[\]/H$\beta$ ratio and weak $\lambda$4686 emission. The very strong \[\]/H$\alpha$ ratio is consistent with the strong nebular bi-polarity [@Shaw_etal06].

[*LMC–RP 671.—*]{}This object is confirmed as an extremely low surface brightness PN. It is very apparent in the combined 5000 s exposure with the WFPC2/F656N filter, but it is barely detected in F450W and F606W images. This nebula is large, nearly perfectly round, and is similar in appearance to many Galactic 