Image Details
Caption: Figure 5.
Comparison of the surface brightness profiles and model fits for NGVS ﹩{g}^{{\prime} }﹩-band and HST/ACS F475W images of NGVS-UCD190—a certain eUCD classified in NGVS. The two-component 1D profile in NGVS is much more clear in HST imaging, thereby strengthening the selection and classification methods of eUCDs.
© 2026. The Author(s). Published by the American Astronomical Society.