Comparison between the stellar mass obtained from SED fitting in the work of W14, and the stellar mass computed as the sum of the value in each pixel of the stellar mass maps created for this work, from the F160W images as explained in Sect. 2.3. The red line is the one-to-one relation. The total stellar mass derived from our resolved stellar mass maps is in very good agreement with the estimate obtained from the integrated photometry (scatter of 0.15 dex).