Similar stellar systems in the Virgo Cluster {#sec:search}
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The optical appearance of AGC 226067 in three-color RGB images, combined with its strong detection in [*GALEX*]{} imaging, is striking [see @Sand15]. Motivated to understand the uniqueness of AGC 226067 we undertook a search of a 20 deg$^2$ region in the Next Generation Virgo cluster Survey (NGVS) footprint to identify similar systems. The NGVS is a $\sim$100 deg$^2$ optical imaging survey conducted with the MegaCam imager on the Canada France Hawaii Telescope (CFHT); details are described in @NGVS. The typical point source depth was $g$$\approx$25.9 mag (10$\sigma$). We downloaded fields from the CFHT archive, utilizing the MegaPipe data products [@Gwyn08], in the rectangular region demarcated by fields \[1,1\] to \[-2,-3\], using the nomenclature presented in Figure 4 of @NGVS. Color RGB images were made with the $u$, $g$ and $i$ band data, and searched by two of us (DJS and DC). We purposely avoided areas directly adjacent to prominent Virgo cluster galaxies, which often have blue, knotty extensions indicative of extended star formation [e.g. @Thilker07] and have a similar appearance as our more isolated examples. [*GALEX*]{} [@GALEX] imaging was used to support our candidate detections.

Two candidates visually similar to AGC 