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 a ect the calculation of first, completeness as a function of image-plane integrated flux density curves for di erent image-plane scale radii; and second, image-plane integrated flux densities estimated for low-significance ALMA detections. These in turn a ect the calculation of deboosting correction factors, demagnified integrated flux densities (for low-significance ALMA detections), di erential and cumulative number counts, and the contribution to the extragalactic background light.
Áreas temáticas de ASJC Scopus
- Astronomía y astrofísica
- Ciencias planetarias y espacial