In this talk I have presented the data analysis results of extracting
properties of halo WIMPs: the mass and the (ratios between the)
spin-independent and spin-dependent couplings/cross sections on nucleons by the
AMIDAS website by taking into account possible unrejected background events in
the analyzed data sets. Although non-standard astronomical setup has been used
to generate pseudodata sets for our analyses, it has been found that, without
prior information/assumption about the local density and velocity distribution
of halo Dark Matter, these WIMP properties have been reconstructed with ~ 2% to
<~ 30% deviations from the input values.Comment: 9 pages, 10 eps figures, 1 table, to appear in the proceedings of the
Seventh International Workshop on the Dark Side of the Universe (DSU 2011),
September 26-30, 2011, Beijing, Chin