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A simple formula is introduced which indicates the amount by which projections of dark matter direct detection experiments are expected to be degraded due to backgrounds.
G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
1996
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P. Benetti et al
2008
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Cited in the paper.
Dark Matter Scientific Assessment Group (DMSAG) http://www.nsf.gov/mps/ast/dmsag.jsp
Cited in the paper.
2008
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