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XENON1T dark matter data analysis: Signal reconstruction, calibration, and event selection
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Nikhef and the University of Amsterdam, Netherlands.
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Number of Authors: 1282019 (English)In: Physical Review D: covering particles, fields, gravitation, and cosmology, ISSN 2470-0010, E-ISSN 2470-0029, Vol. 100, no 5, article id 052014Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2019. Vol. 100, no 5, article id 052014
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Physical Sciences
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URN: urn:nbn:se:su:diva-174921DOI: 10.1103/PhysRevD.100.052014ISI: 000487731600001OAI: oai:DiVA.org:su-174921DiVA, id: diva2:1360694
Available from: 2019-10-14 Created: 2019-10-14 Last updated: 2019-12-04Bibliographically approved

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Aalbers, JelleAntochi, Vasile CristianBauermeister, BorisConrad, JanFerella, Alfredo D.Mahlstedt, JörnMorå, KnutPelssers, Bart
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