Fig. 7.
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Baryonic mass vs. outermost rotational velocity. MIGHTEE galaxies are shown with magenta circles, with galaxies from the COSMOS field (not searched for LSBG/UDGs) in a lighter magenta. The four galaxies of this work (meeting both LSBG and UDG classification criteria) are shown as blue diamonds. The derived bTFr from Ponomareva et al. (2021) is shown by the black line.
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