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Fig. 5.

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Stellar-to-halo mass ratio, specific angular momentum, sSFR, and H I+H2 fraction as functions of stellar mass. Grey regions and grey solid lines indicate the 20th − 80th percentile range and median values for the PS sample, respectively. Horizontal lines correspond to median values as the legend indicates. For reference, Milky-Way estimates are included, based on analytic models calibrated to observations from Gaia DR2, VERA, and APOGEE. BL galaxies typically reside in lower-mass dark matter haloes, exhibit higher specific angular momentum, H I+H2 gas fractions, and star formation rates than their BD counterparts.

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