Ratio of effective radius in different bands to effective radius in FIR measured by fitting a single Gaussian to our original ALMA stacked images. Yellow, brown, and pink circles correspond the optical size measured from the HST i-band, UltraVISTA J-band, and UltraVISTA K_s-band light profiles, respectively. Blue squares display the FIR size measured from the ALMA light profile. Brown stars show the stellar mass effective radius inferred by correcting our UltraVISTA J-band sizes with a R_{half-stellar-light}-to-R_{half-stellar-mass} relation at rest 5000 Å from Suess et al. (2019). We provide lower limits of the size ratio in the highest ΔMS and 10^10.0 ≤ M_★ /M_⊙ < 10^10.5 bin because these galaxies are unresolved in our ALMA stacked images. The maximun value of ΔMS for the mid-low, mid-high, and high stellar mass bin are 0.9, 1.0, and 1.1; and the minimum value for the mid-low, mid-high, and high stellar mass bin are −0.7, −0.7, and −0.6, respectively.