226067 were identified, and are shown in Figure \[fig:newobjects\]. Each is characterized by an over-density of compact blue sources with strong GALEX UV emission. The objects also lack a diffuse reddish galaxy component, exhibited by dwarf galaxies throughout the NGVS imaging. Aperture photometry [@Sand14] is reported for each object in Table \[table:properties\]; the objects are of similar brightness as AGC 226067 in the $NUV,g$ bands to within the uncertainties [@Sand15]. We searched for HI counterparts to our newly identified blue stellar systems using the 40% ALFALFA catalog [@Haynes11]. No catalogued HI counterparts were found to either source within $\sim$10’, and a visual inspection of the ALFALFA data did not turn up any marginal detections. Assuming that these objects are similar to AGC 226067, with D=17 Mpc and velocity width $\sim$50 km s$^{-1}$, we estimate an HI limiting mass of $\sim$2$\times$10$^7$ $M_{\odot}$ for each. AGC 226067 itself has an $M_{HI}$$\approx$5$\times$10$^7$ $M_{\odot}$ in the ALFALFA catalog, so a similar HI cloud with a slightly higher distance and/or velocity width would not be detectable with the ALFALFA data. We also note that ALFALFA is blind to emission that spectrally overlaps with the Galactic HI layer at $-$100 $\lesssim$ $v_{lsr}$ (km s$^{-1})$ $\lesssim$ 100 