摘要：We noticed an error in the code that conducts the source injection
simulations used in our article Muñoz Arancibia et al. (2018).
This error led the source scale radii in the image plane to be
1=2:35 times smaller that what it should be. Wrongly computed
scale radii primarily affect the calculation of first, completeness as a function of image-plane integrated flux density curves
for different image-plane scale radii; and second, image-plane
integrated flux densities estimated for low-significance ALMA
detections. These in turn affect the calculation of deboosting
correction factors, demagnified integrated flux densities (for
low-significance ALMA detections), differential and cumulative
number counts, and the contribution to the extragalactic background light.
