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Fig. G.5

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Image gallery of a selection of spurious UV source detections between the SDSS and NGVS i-band limits in Fig. G.2, which are sources with UV Kron aperture semi-major axis <10′′. Each line of the two columns shows the GALEX NUV, NGVS g-band, NGVS i-band, and NGVS z-band images. The magnitudes in each band are listed at the top of each stamp, and the VPS_ID is listed vertically along the right edge of the z-band image. The cyan apertures are the NUV Kron apertures automatically calculated in the GALEX pipeline.

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