Figure taken from Hennebelle & Grudić (2024) review on the IMF overlapped with the parametrisation of the mean-normalised IMF based on our detections (blue lines and shaded region) and the S_lit members (black lines and shaded region). The plot shows the slope of different estimation of the IMFs of several populations in the Milky Way disc as a function of the stellar mass from the literature. The shadowed region corresponds to the propagated errors in the estimation of the parameters of the mean-normalised IMF of the NYMGs.