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A 20 arcmin \times 20 arcmin region around 30 Doradus in the Large MagellanicCloud (LMC) is observed and analyzed in the near-infrared. We obtainpolarimetry data in the J, H, and K_s bands using the SIRIUS polarimeter SIRPOLat the Infrared Survey Facility 1.4 m telescope. We measure the Stokesparameters of 2562 point-like sources to derive the degree of polarization andthe polarization position angles. We discuss the statistics of the groupsclassified by color-magnitude diagram and proper motions of the sources, inorder to separate the Galactic foreground sources from those present in theLMC. We notice that groups classified by the proper motion data show a tendencytowards different polarimetric properties.

Near-IR Polarimetry Around 30 Doradus: I. Separation of the Galactic Sources