4.7 Article

XENON1T dark matter data analysis: Signal reconstruction, calibration, and event selection

期刊

PHYSICAL REVIEW D
卷 100, 期 5, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.100.052014

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资金

  1. National Science Foundation
  2. Swiss National Science Foundation
  3. German Ministry for Education and Research
  4. Max Planck Gesellschaft
  5. Deutsche Forschungsgemeinschaft
  6. Netherlands Organisation for Scientic Research (NWO)
  7. Netherlands eScience Center (NLeSC)
  8. SURF Cooperative
  9. Weizmann Institute of Science
  10. Israeli Centers Of Research Excellence (I-CORE)
  11. Pazy-Vatat
  12. Initial Training Network Invisibles (Marie Curie Actions) [PITNGA-2011-289442]
  13. Fundacao para a Ciencia e a Tecnologia
  14. Region des Pays de la Loire
  15. Knut and Alice Wallenberg Foundation
  16. Kavli Foundation
  17. Istituto Nazionale di Fisica Nucleare
  18. Laboratori Nazionali del Gran Sasso

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The XENON1T experiment at the Laboratori Nazionali del Gran Sasso is the most sensitive direct detection experiment for dark matter in the form of weakly interacting particles (WIMPs) with masses above 6 GeV/c(2) scattering off nuclei. The detector employs a dual-phase time projection chamber with 2.0 metric tons of liquid xenon in the target. A one metric ton x year exposure of science data was collected between October 2016 and February 2018. This article reports on the performance of the detector during this period and describes details of the data analysis that led to the most stringent exclusion limits on various WIMP-nucleon interaction models to date. In particular, signal reconstruction, event selection, and calibration of the detector response to nuclear and electronic recoils in XENON1T are discussed.

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