Stellar mass dependent galaxy size-dark matter halo radius relation unveiled by Subaru-HSC survey weak lensing measurements

We investigate the stellar mass-dependence of the galaxy size-dark matter halo radius relation for low redshift galaxies using weak gravitational lensing measurements. Our sample consists of $\sim$38,000 galaxies more massive than $10^{8} {\rm M}_{\odot}h^{-2}$ and within $z
19 pages, 11 figures, submitted to the MNRAS