Extended Data 2: Distribution of the Mdyn-to-Mbary ratio with different misalignments between optical image and H i velocity field.
From: Further evidence for a population of dark-matter-deficient dwarf galaxies
a, The distribution of the misalignment between optical image and H i velocity field for dwarf galaxies in LITTLE THINGS(red)/Illustris(cyan). b,c, Distribution of the Mdyn/Mbary ratio for our parent sample after applying the same distribution of misalignment between optical image and H i velocity field from the LITTLE THINGS/Illustris in the left panel. Grey histogram is based on 10,000 random realizations and black curve is the Gaussian fit. Samples classified as BDDGs are highlighted with blue histogram.
