1005 galaxies with z<0.09 sample

Taking advantage of this situation, we define a new physically motivated measurement of size for galaxies based on the expected location of the gas density threshold for star formation. Employing both theoretical and observational arguments, we use the stellar mass density contour at 1M_{sun}/pc^2^ as a proxy for this density threshold for star formation.

This choice makes our size definition operative. With this new size measure, the intrinsic scatter of the global stellar mass (M*)-size relation (explored over five orders of magnitude in stellar mass) decreases to ~0.06dex. This value is 2.5 times smaller than the scatter measured using the effective radius (~0.15dex) and between 1.5 and 1.8 times smaller than those using other traditional size indicators such as R_23.5,i_ (~0.09dex), the Holmberg radius RH (~0.09dex), and the half-mass radius R_e,M*_ (~0.11dex).