Issue |
EAS Publications Series
Volume 53, 2012
CYGNUS 2011: Third International Conference on Directional Detection of Dark Matter
|
|
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Page(s) | 77 - 88 | |
DOI | https://doi.org/10.1051/eas/1253010 | |
Published online | 15 February 2012 |
F. Mayet and D. Santos (eds)
EAS Publications Series, 53 (2012) 77-88
Analyzing Direct Dark Matter Detection Data by the AMIDAS Website
Institute of Physics, Academia
Sinica, No. 128, Sec. 2, Academia
Road, Nankang, Taipei
11529, Taiwan,
R.O.C. ;
e-mail: clshan@phys.sinica.edu.tw
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. 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 ~5% to ≲40% deviations from the input values.
© EAS, EDP Sciences 2012