European Physical Journal C: Particles and Fields (Jun 2023)

Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source

  • E. Aprile,
  • K. Abe,
  • F. Agostini,
  • S. Ahmed Maouloud,
  • M. Alfonsi,
  • L. Althueser,
  • B. Andrieu,
  • E. Angelino,
  • J. R. Angevaare,
  • V. C. Antochi,
  • D. Antón Martin,
  • F. Arneodo,
  • L. Baudis,
  • A. L. Baxter,
  • L. Bellagamba,
  • R. Biondi,
  • A. Bismark,
  • A. Brown,
  • S. Bruenner,
  • G. Bruno,
  • R. Budnik,
  • T. K. Bui,
  • C. Cai,
  • C. Capelli,
  • J. M. R. Cardoso,
  • D. Cichon,
  • A. P. Colijn,
  • J. Conrad,
  • J. J. Cuenca-García,
  • J. P. Cussonneau,
  • V. D’Andrea,
  • M. P. Decowski,
  • P. Di Gangi,
  • S. Di Pede,
  • S. Diglio,
  • K. Eitel,
  • A. Elykov,
  • S. Farrell,
  • A. D. Ferella,
  • C. Ferrari,
  • H. Fischer,
  • W. Fulgione,
  • P. Gaemers,
  • R. Gaior,
  • A. Gallo Rosso,
  • M. Galloway,
  • F. Gao,
  • R. Glade-Beucke,
  • L. Grandi,
  • J. Grigat,
  • M. Guida,
  • R. Hammann,
  • A. Higuera,
  • C. Hils,
  • L. Hoetzsch,
  • J. Howlett,
  • M. Iacovacci,
  • Y. Itow,
  • J. Jakob,
  • F. Joerg,
  • A. Joy,
  • N. Kato,
  • M. Kara,
  • P. Kavrigin,
  • S. Kazama,
  • M. Kobayashi,
  • G. Koltman,
  • A. Kopec,
  • F. Kuger,
  • H. Landsman,
  • R. F. Lang,
  • L. Levinson,
  • I. Li,
  • S. Li,
  • S. Liang,
  • S. Lindemann,
  • M. Lindner,
  • K. Liu,
  • J. Loizeau,
  • F. Lombardi,
  • J. Long,
  • J. A. M. Lopes,
  • Y. Ma,
  • C. Macolino,
  • J. Mahlstedt,
  • A. Mancuso,
  • L. Manenti,
  • F. Marignetti,
  • T. Marrodán Undagoitia,
  • K. Martens,
  • J. Masbou,
  • D. Masson,
  • E. Masson,
  • S. Mastroianni,
  • M. Messina,
  • K. Miuchi,
  • K. Mizukoshi,
  • A. Molinario,
  • S. Moriyama,
  • K. Morå,
  • Y. Mosbacher,
  • M. Murra,
  • J. Müller,
  • K. Ni,
  • U. Oberlack,
  • B. Paetsch,
  • J. Palacio,
  • R. Peres,
  • C. Peters,
  • J. Pienaar,
  • M. Pierre,
  • V. Pizzella,
  • G. Plante,
  • J. Qi,
  • J. Qin,
  • D. Ramírez García,
  • S. Reichard,
  • A. Rocchetti,
  • N. Rupp,
  • L. Sanchez,
  • P. Sanchez-Lucas,
  • J. M. F. dos Santos,
  • I. Sarnoff,
  • G. Sartorelli,
  • J. Schreiner,
  • D. Schulte,
  • P. Schulte,
  • H. Schulze Eißing,
  • M. Schumann,
  • L. Scotto Lavina,
  • M. Selvi,
  • F. Semeria,
  • P. Shagin,
  • S. Shi,
  • E. Shockley,
  • M. Silva,
  • H. Simgen,
  • A. Takeda,
  • P.-L. Tan,
  • A. Terliuk,
  • D. Thers,
  • F. Toschi,
  • G. Trinchero,
  • C. Tunnell,
  • F. Tönnies,
  • K. Valerius,
  • G. Volta,
  • C. Weinheimer,
  • M. Weiss,
  • D. Wenz,
  • C. Wittweg,
  • T. Wolf,
  • D. Xu,
  • Z. Xu,
  • M. Yamashita,
  • L. Yang,
  • J. Ye,
  • L. Yuan,
  • G. Zavattini,
  • S. Zerbo,
  • M. Zhong,
  • T. Zhu,
  • C. Geppert,
  • J. Riemer,
  • XENON Collaboration

DOI
https://doi.org/10.1140/epjc/s10052-023-11512-z
Journal volume & issue
Vol. 83, no. 6
pp. 1 – 15

Abstract

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Abstract A low-energy electronic recoil calibration of XENON1T, a dual-phase xenon time projection chamber, with an internal $${}^{37}$$ 37 Ar source was performed. This calibration source features a 35-day half-life and provides two mono-energetic lines at 2.82 keV and 0.27 keV. The photon yield and electron yield at 2.82 keV are measured to be ( $$32.3\,\pm \,0.3$$ 32.3 ± 0.3 ) photons/keV and ( $$40.6\,\pm \,0.5$$ 40.6 ± 0.5 ) electrons/keV, respectively, in agreement with other measurements and with NEST predictions. The electron yield at 0.27 keV is also measured and it is ( $$68.0^{+6.3}_{-3.7}$$ 68 . 0 - 3.7 + 6.3 ) electrons/keV. The $${}^{37}$$ 37 Ar calibration confirms that the detector is well-understood in the energy region close to the detection threshold, with the 2.82 keV line reconstructed at ( $$2.83\,\pm \,0.02$$ 2.83 ± 0.02 ) keV, which further validates the model used to interpret the low-energy electronic recoil excess previously reported by XENON1T. The ability to efficiently remove argon with cryogenic distillation after the calibration proves that $${}^{37}$$ 37 Ar can be considered as a regular calibration source for multi-tonne xenon detectors.