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The Magellanic Clouds offer a unique variety of star forming regions seen asbright nebulae of ionized gas, related to bright young stellar associations.Nowadays, observations with the high resolving efficiency of the Hubble SpaceTelescope allow the detection of the faintest infant stars, and a more completepicture of clustered star formation in our dwarf neighbors has emerged. Ipresent results from our studies of the Magellanic Clouds, with emphasis in theyoung low-mass pre-main sequence populations. Our data include imaging with theAdvanced Camera for Surveys of the association LH~95 in the Large MagellanicCloud, the deepest observations ever taken with HST of this galaxy. I discussour findings in terms of the Initial Mass Function, which we constructed withan unprecedented completeness down to the sub-solar regime, as the outcome ofstar formation in the low-metallicity environment of the LMC.

The sub-solar Initial Mass Function in the Large Magellanic Cloud