Fig. 7.
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Zoom-in SHMR for our galaxy sample contrasted against estimates from weak lensing (Dvornik et al. 2020; Luo et al. 2022; Thornton et al. 2024). For the lensing data, vertical error bars represent the width of the M* bin of each measurement. The independent results from weak lensing and rotation curve decomposition suggest the existence of a population of BDDs. Note the smaller mass span compared to Fig. 6.
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