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
Affiliations
- E. Aprile
- Physics Department, Columbia University
- K. Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- F. Agostini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- S. Ahmed Maouloud
- LPNHE, Sorbonne Université, CNRS/IN2P3
- M. Alfonsi
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- L. Althueser
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- B. Andrieu
- LPNHE, Sorbonne Université, CNRS/IN2P3
- E. Angelino
- INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino
- J. R. Angevaare
- Nikhef and the University of Amsterdam
- V. C. Antochi
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- D. Antón Martin
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- F. Arneodo
- New York University Abu Dhabi, Center for Astro, Particle and Planetary Physics
- L. Baudis
- Physik-Institut, University of Zürich
- A. L. Baxter
- Department of Physics and Astronomy, Purdue University
- L. Bellagamba
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- R. Biondi
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- A. Bismark
- Physik-Institut, University of Zürich
- A. Brown
- Physikalisches Institut, Universität Freiburg
- S. Bruenner
- Nikhef and the University of Amsterdam
- G. Bruno
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- R. Budnik
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- T. K. Bui
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- C. Cai
- Department of Physics, Center for High Energy Physics, Tsinghua University
- C. Capelli
- Physik-Institut, University of Zürich
- J. M. R. Cardoso
- LIBPhys, Department of Physics, University of Coimbra
- D. Cichon
- Max-Planck-Institut für Kernphysik
- A. P. Colijn
- Nikhef and the University of Amsterdam
- J. Conrad
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- J. J. Cuenca-García
- Physik-Institut, University of Zürich
- J. P. Cussonneau
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- V. D’Andrea
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- M. P. Decowski
- Nikhef and the University of Amsterdam
- P. Di Gangi
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- S. Di Pede
- Nikhef and the University of Amsterdam
- S. Diglio
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- K. Eitel
- Institute for Astroparticle Physics, Karlsruhe Institute of Technology
- A. Elykov
- Physikalisches Institut, Universität Freiburg
- S. Farrell
- Department of Physics and Astronomy, Rice University
- A. D. Ferella
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- C. Ferrari
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- H. Fischer
- Physikalisches Institut, Universität Freiburg
- W. Fulgione
- INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino
- P. Gaemers
- Nikhef and the University of Amsterdam
- R. Gaior
- LPNHE, Sorbonne Université, CNRS/IN2P3
- A. Gallo Rosso
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- M. Galloway
- Physik-Institut, University of Zürich
- F. Gao
- Department of Physics, Center for High Energy Physics, Tsinghua University
- R. Glade-Beucke
- Physikalisches Institut, Universität Freiburg
- L. Grandi
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- J. Grigat
- Physikalisches Institut, Universität Freiburg
- M. Guida
- Max-Planck-Institut für Kernphysik
- R. Hammann
- Max-Planck-Institut für Kernphysik
- A. Higuera
- Department of Physics and Astronomy, Rice University
- C. Hils
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- L. Hoetzsch
- Max-Planck-Institut für Kernphysik
- J. Howlett
- Physics Department, Columbia University
- M. Iacovacci
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- Y. Itow
- Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya University
- J. Jakob
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- F. Joerg
- Max-Planck-Institut für Kernphysik
- A. Joy
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- N. Kato
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- M. Kara
- Institute for Astroparticle Physics, Karlsruhe Institute of Technology
- P. Kavrigin
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- S. Kazama
- Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya University
- M. Kobayashi
- Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya University
- G. Koltman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- A. Kopec
- Department of Physics, University of California San Diego
- F. Kuger
- Physikalisches Institut, Universität Freiburg
- H. Landsman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- R. F. Lang
- Department of Physics and Astronomy, Purdue University
- L. Levinson
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- I. Li
- Department of Physics and Astronomy, Rice University
- S. Li
- Department of Physics and Astronomy, Purdue University
- S. Liang
- Department of Physics and Astronomy, Rice University
- S. Lindemann
- Physikalisches Institut, Universität Freiburg
- M. Lindner
- Max-Planck-Institut für Kernphysik
- K. Liu
- Department of Physics, Center for High Energy Physics, Tsinghua University
- J. Loizeau
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- F. Lombardi
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- J. Long
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- J. A. M. Lopes
- LIBPhys, Department of Physics, University of Coimbra
- Y. Ma
- Department of Physics, University of California San Diego
- C. Macolino
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- J. Mahlstedt
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- A. Mancuso
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- L. Manenti
- New York University Abu Dhabi, Center for Astro, Particle and Planetary Physics
- F. Marignetti
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- T. Marrodán Undagoitia
- Max-Planck-Institut für Kernphysik
- K. Martens
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- J. Masbou
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- D. Masson
- Physikalisches Institut, Universität Freiburg
- E. Masson
- LPNHE, Sorbonne Université, CNRS/IN2P3
- S. Mastroianni
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- M. Messina
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- K. Miuchi
- Department of Physics, Kobe University
- K. Mizukoshi
- Department of Physics, Kobe University
- A. Molinario
- INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino
- S. Moriyama
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- K. Morå
- Physics Department, Columbia University
- Y. Mosbacher
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- M. Murra
- Physics Department, Columbia University
- J. Müller
- Physikalisches Institut, Universität Freiburg
- K. Ni
- Department of Physics, University of California San Diego
- U. Oberlack
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- B. Paetsch
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- J. Palacio
- Max-Planck-Institut für Kernphysik
- R. Peres
- Physik-Institut, University of Zürich
- C. Peters
- Department of Physics and Astronomy, Rice University
- J. Pienaar
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- M. Pierre
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- V. Pizzella
- Max-Planck-Institut für Kernphysik
- G. Plante
- Physics Department, Columbia University
- J. Qi
- Department of Physics, University of California San Diego
- J. Qin
- Department of Physics and Astronomy, Purdue University
- D. Ramírez García
- Physik-Institut, University of Zürich
- S. Reichard
- Institute for Astroparticle Physics, Karlsruhe Institute of Technology
- A. Rocchetti
- Physikalisches Institut, Universität Freiburg
- N. Rupp
- Max-Planck-Institut für Kernphysik
- L. Sanchez
- Department of Physics and Astronomy, Rice University
- P. Sanchez-Lucas
- Physik-Institut, University of Zürich
- J. M. F. dos Santos
- LIBPhys, Department of Physics, University of Coimbra
- I. Sarnoff
- New York University Abu Dhabi, Center for Astro, Particle and Planetary Physics
- G. Sartorelli
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- J. Schreiner
- Max-Planck-Institut für Kernphysik
- D. Schulte
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- P. Schulte
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- H. Schulze Eißing
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- M. Schumann
- Physikalisches Institut, Universität Freiburg
- L. Scotto Lavina
- LPNHE, Sorbonne Université, CNRS/IN2P3
- M. Selvi
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- F. Semeria
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- P. Shagin
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- S. Shi
- Physics Department, Columbia University
- E. Shockley
- Department of Physics, University of California San Diego
- M. Silva
- LIBPhys, Department of Physics, University of Coimbra
- H. Simgen
- Max-Planck-Institut für Kernphysik
- A. Takeda
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- P.-L. Tan
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- A. Terliuk
- Max-Planck-Institut für Kernphysik
- D. Thers
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- F. Toschi
- Physikalisches Institut, Universität Freiburg
- G. Trinchero
- INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino
- C. Tunnell
- Department of Physics and Astronomy, Rice University
- F. Tönnies
- Physikalisches Institut, Universität Freiburg
- K. Valerius
- Institute for Astroparticle Physics, Karlsruhe Institute of Technology
- G. Volta
- Physik-Institut, University of Zürich
- C. Weinheimer
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- M. Weiss
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- D. Wenz
- Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität Mainz
- C. Wittweg
- Physik-Institut, University of Zürich
- T. Wolf
- Max-Planck-Institut für Kernphysik
- D. Xu
- Physics Department, Columbia University
- Z. Xu
- Physics Department, Columbia University
- M. Yamashita
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo
- L. Yang
- Department of Physics, University of California San Diego
- J. Ye
- Physics Department, Columbia University
- L. Yuan
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- G. Zavattini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- S. Zerbo
- Physics Department, Columbia University
- M. Zhong
- Department of Physics, University of California San Diego
- T. Zhu
- Physics Department, Columbia University
- C. Geppert
- Forschungsreaktor TRIGA Mainz, Johannes Gutenberg-Universität Mainz
- J. Riemer
- Forschungsreaktor TRIGA Mainz, Johannes Gutenberg-Universität Mainz
- XENON Collaboration
- DOI
- https://doi.org/10.1140/epjc/s10052-023-11512-z
- Journal volume & issue
-
Vol. 83,
no. 6
pp. 1 – 15
Abstract
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.