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In this paper, we revisit our model-independent methods developed forreconstructing properties of Weakly Interacting Massive Particles (WIMPs) byusing measured recoil energies from direct Dark Matter detection experimentsdirectly and take into account more realistically non-negligible thresholdenergy. All expressions for reconstructing the mass and the (ratios betweenthe) spin-independent and the spin-dependent WIMP-nucleon couplings have beenmodified. We focus on low-mass (m_chi <~ 15 GeV) WIMPs and present thenumerical results obtained by Monte Carlo simulations. Constraints caused bynon-negligible threshold energy and technical treatments for improvingreconstruction results will also be discussed.

Effects of Threshold Energy on Reconstructions of Properties of Low-Mass WIMPs in Direct Dark Matter Detection Experiments