Relative detection frequency due to extinction versus projected distance to Sgr A*, in pointing 1 for min_correlation = 0.8 and deblend = 0. The blue crosses give the values of p for each magnitude bin. The green line represents the mean of the p(%) considering detected stars at the same distance from Sgr A*. We can observe that for close distances to Sgr A*p(%) is higher than for large distances, as we expected, because the extinction near Sg A* is lower.