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Performance data from the ZEPLIN-III second science run
Preprint
P. Majewski ,
V. N. Solovov ,
D. Yu. Akimov ,
H. M. Araujo ,
E. J. Barnes ,
V. A. Belov ,
A. A. Burenkov ,
V. Chepel ,
A. Currie ,
L. DeViveiros ,
B. Edwards ,
C. Ghag ,
A. Hollingsworth ,
M. Horn ,
G. E. Kalmus ,
A. S. Kobyakin ,
A. G. Kovalenko ,
V. N. Lebedenko ,
A. Lindote ,
M. I. Lopes ,
R. Luscher ,
A. St J. Murphy ,
F. Neves ,
S. M. Paling ,
J. Pinto da Cunha ,
R. Preece ,
J. J. Quenby ,
L. Reichhart ,
P. R. Scovell ,
C. Silva ,
N. J. T. Smith ,
V. N. Stekhanov ,
T. J. Sumner ,
C. Thorne ,
R. J. Walker
30 November 2011
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Abstract
ZEPLIN-III is a two-phase xenon direct dark matter experiment located at the Boulby Mine (UK). After its first science run in 2008 it was upgraded with: an array of low background photomultipliers, a new anti-coincidence detector system with plastic scintillator and an improved calibration system. After 319 days of data taking the second science run ended in May 2011. In this paper we describe the instrument performance with emphasis on the position and energy reconstruction algorithm and summarise the final science results.
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Most cited references3
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First limits on nuclear recoil events from the ZEPLIN I galactic dark matter detector
G.J. Alner, H Araujo, G.J. Arnison … (2005)
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Maximum a Posteriori Estimation of Position in Scintillation Cameras
Robert M. Gray, Albert Macovski (1976)