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- Gaitskell, RJ;
- Gehman, VM;
- Ghag, C;
- Gibson, KR;
- Gilchriese, MGD;
- Hall, C;
- Hanhardt, M;
- Haselschwardt, S;
- Hertel, SA;
- Huang, DQ;
- Ihm, M;
- Jacobsen, RG;
- Kazkaz, K;
- Knoche, R;
- Larsen, NA;
- Lee, C;
- Lenardo, B;
- Lesko, KT;
- Lindote, A;
- Lopes, MI;
- Malling, DC;
- Mannino, R;
- McKinsey, DN;
- Mei, D-M;
- Mock, J;
- Moongweluwan, M;
- Morad, J;
- Murphy;
- Nehrkorn, C;
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- Parker, PD;
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- Collaboration, On behalf of the LUX
© 2014 Elsevier B.V. The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370. kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. First results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.