Journal
PHYSICAL REVIEW D
Volume 96, Issue 11, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.96.112009
Keywords
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Funding
- U.S. Department of Energy (DOE) [DE-AC02-05CH11231, DE-AC05-06OR23100, DE-AC52-07NA27344, DE-FG01-91ER40618, DE-FG02-08ER41549, DE-FG02-11ER41738, DE-FG02-91ER40674, DE-FG02-91ER40688, DE-FG02-95ER40917, DE-NA0000979, DE-SC0006605, DE-SC0010010, DE-SC0015535]
- U.S. National Science Foundation [PHY-0750671, PHY-0801536, PHY-1003660, PHY-1004661, PHY-1102470, PHY-1312561, PHY-1347449, PHY-1505868, PHY-1636738]
- Research Corporation [RA0350]
- Center for Ultra-low Background Experiments in the Dakotas (CUBED)
- South Dakota School of Mines and Technology (SDSMT)
- Fundacao para a Ciencia e a Tecnologia (FCT) [PTDC/FIS-NUC/1525/2014]
- U.K. Royal Society [IE120804]
- Science and Technology Facilities Council [ST/K502042/1, ST/K502406/1, ST/M503538/1]
- STFC [ST/K502042/1, ST/N000242/1, ST/K003208/1, ST/K502406/1, ST/M003744/1, ST/M503538/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/M503538/1, ST/K003208/1, ST/N000242/1, ST/K003208/1 DMUK, ST/K502406/1, ST/K502042/1] Funding Source: researchfish
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LUX was the first dark matter experiment to use a Kr-83m calibration source. In this paper, we describe the source preparation and injection. We also present several Kr-83m calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.
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