Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source
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 an...
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2023-06-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-023-11512-z |
| _version_ | 1827894894141636608 |
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| author | 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 |
| author_facet | 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 |
| author_sort | E. Aprile |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-03-12T22:14:12Z |
| format | Article |
| id | doaj.art-637738a0b4d6429daf9ce87987ac4536 |
| institution | Directory Open Access Journal |
| issn | 1434-6052 |
| language | English |
| last_indexed | 2024-03-12T22:14:12Z |
| publishDate | 2023-06-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj.art-637738a0b4d6429daf9ce87987ac45362023-07-23T11:23:48ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-06-0183611510.1140/epjc/s10052-023-11512-zLow-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar sourceE. Aprile0K. Abe1F. Agostini2S. Ahmed Maouloud3M. Alfonsi4L. Althueser5B. Andrieu6E. Angelino7J. R. Angevaare8V. C. Antochi9D. Antón Martin10F. Arneodo11L. Baudis12A. L. Baxter13L. Bellagamba14R. Biondi15A. Bismark16A. Brown17S. Bruenner18G. Bruno19R. Budnik20T. K. Bui21C. Cai22C. Capelli23J. M. R. Cardoso24D. Cichon25A. P. Colijn26J. Conrad27J. J. Cuenca-García28J. P. Cussonneau29V. D’Andrea30M. P. Decowski31P. Di Gangi32S. Di Pede33S. Diglio34K. Eitel35A. Elykov36S. Farrell37A. D. Ferella38C. Ferrari39H. Fischer40W. Fulgione41P. Gaemers42R. Gaior43A. Gallo Rosso44M. Galloway45F. Gao46R. Glade-Beucke47L. Grandi48J. Grigat49M. Guida50R. Hammann51A. Higuera52C. Hils53L. Hoetzsch54J. Howlett55M. Iacovacci56Y. Itow57J. Jakob58F. Joerg59A. Joy60N. Kato61M. Kara62P. Kavrigin63S. Kazama64M. Kobayashi65G. Koltman66A. Kopec67F. Kuger68H. Landsman69R. F. Lang70L. Levinson71I. Li72S. Li73S. Liang74S. Lindemann75M. Lindner76K. Liu77J. Loizeau78F. Lombardi79J. Long80J. A. M. Lopes81Y. Ma82C. Macolino83J. Mahlstedt84A. Mancuso85L. Manenti86F. Marignetti87T. Marrodán Undagoitia88K. Martens89J. Masbou90D. Masson91E. Masson92S. Mastroianni93M. Messina94K. Miuchi95K. Mizukoshi96A. Molinario97S. Moriyama98K. Morå99Y. Mosbacher100M. Murra101J. Müller102K. Ni103U. Oberlack104B. Paetsch105J. Palacio106R. Peres107C. Peters108J. Pienaar109M. Pierre110V. Pizzella111G. Plante112J. Qi113J. Qin114D. Ramírez García115S. Reichard116A. Rocchetti117N. Rupp118L. Sanchez119P. Sanchez-Lucas120J. M. F. dos Santos121I. Sarnoff122G. Sartorelli123J. Schreiner124D. Schulte125P. Schulte126H. Schulze Eißing127M. Schumann128L. Scotto Lavina129M. Selvi130F. Semeria131P. Shagin132S. Shi133E. Shockley134M. Silva135H. Simgen136A. Takeda137P.-L. Tan138A. Terliuk139D. Thers140F. Toschi141G. Trinchero142C. Tunnell143F. Tönnies144K. Valerius145G. Volta146C. Weinheimer147M. Weiss148D. Wenz149C. Wittweg150T. Wolf151D. Xu152Z. Xu153M. Yamashita154L. Yang155J. Ye156L. Yuan157G. Zavattini158S. Zerbo159M. Zhong160T. Zhu161C. Geppert162J. Riemer163XENON CollaborationPhysics Department, Columbia UniversityKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaLPNHE, Sorbonne Université, CNRS/IN2P3Institut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterLPNHE, Sorbonne Université, CNRS/IN2P3INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-TorinoNikhef and the University of AmsterdamDepartment of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaDepartment of Physics, Kavli Institute for Cosmological Physics, University of ChicagoNew York University Abu Dhabi, Center for Astro, Particle and Planetary PhysicsPhysik-Institut, University of ZürichDepartment of Physics and Astronomy, Purdue UniversityDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstitutePhysik-Institut, University of ZürichPhysikalisches Institut, Universität FreiburgNikhef and the University of AmsterdamSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoDepartment of Physics, Center for High Energy Physics, Tsinghua UniversityPhysik-Institut, University of ZürichLIBPhys, Department of Physics, University of CoimbraMax-Planck-Institut für KernphysikNikhef and the University of AmsterdamDepartment of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaPhysik-Institut, University of ZürichSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstituteNikhef and the University of AmsterdamDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaNikhef and the University of AmsterdamSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesInstitute for Astroparticle Physics, Karlsruhe Institute of TechnologyPhysikalisches Institut, Universität FreiburgDepartment of Physics and Astronomy, Rice UniversityINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstituteINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstitutePhysikalisches Institut, Universität FreiburgINAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-TorinoNikhef and the University of AmsterdamLPNHE, Sorbonne Université, CNRS/IN2P3Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaPhysik-Institut, University of ZürichDepartment of Physics, Center for High Energy Physics, Tsinghua UniversityPhysikalisches Institut, Universität FreiburgDepartment of Physics, Kavli Institute for Cosmological Physics, University of ChicagoPhysikalisches Institut, Universität FreiburgMax-Planck-Institut für KernphysikMax-Planck-Institut für KernphysikDepartment of Physics and Astronomy, Rice UniversityInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzMax-Planck-Institut für KernphysikPhysics Department, Columbia UniversityDepartment of Physics “Ettore Pancini”, University of Napoli and INFN-NapoliKobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya UniversityInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterMax-Planck-Institut für KernphysikDepartment of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoInstitute for Astroparticle Physics, Karlsruhe Institute of TechnologyDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceKobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya UniversityKobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya UniversityDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceDepartment of Physics, University of California San DiegoPhysikalisches Institut, Universität FreiburgDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceDepartment of Physics and Astronomy, Purdue UniversityDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceDepartment of Physics and Astronomy, Rice UniversityDepartment of Physics and Astronomy, Purdue UniversityDepartment of Physics and Astronomy, Rice UniversityPhysikalisches Institut, Universität FreiburgMax-Planck-Institut für KernphysikDepartment of Physics, Center for High Energy Physics, Tsinghua UniversitySUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzDepartment of Physics, Kavli Institute for Cosmological Physics, University of ChicagoLIBPhys, Department of Physics, University of CoimbraDepartment of Physics, University of California San DiegoINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstituteDepartment of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaNew York University Abu Dhabi, Center for Astro, Particle and Planetary PhysicsDepartment of Physics “Ettore Pancini”, University of Napoli and INFN-NapoliMax-Planck-Institut für KernphysikKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesPhysikalisches Institut, Universität FreiburgLPNHE, Sorbonne Université, CNRS/IN2P3Department of Physics “Ettore Pancini”, University of Napoli and INFN-NapoliINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstituteDepartment of Physics, Kobe UniversityDepartment of Physics, Kobe UniversityINAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-TorinoKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoPhysics Department, Columbia UniversityDepartment of Particle Physics and Astrophysics, Weizmann Institute of SciencePhysics Department, Columbia UniversityPhysikalisches Institut, Universität FreiburgDepartment of Physics, University of California San DiegoInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceMax-Planck-Institut für KernphysikPhysik-Institut, University of ZürichDepartment of Physics and Astronomy, Rice UniversityDepartment of Physics, Kavli Institute for Cosmological Physics, University of ChicagoSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesMax-Planck-Institut für KernphysikPhysics Department, Columbia UniversityDepartment of Physics, University of California San DiegoDepartment of Physics and Astronomy, Purdue UniversityPhysik-Institut, University of ZürichInstitute for Astroparticle Physics, Karlsruhe Institute of TechnologyPhysikalisches Institut, Universität FreiburgMax-Planck-Institut für KernphysikDepartment of Physics and Astronomy, Rice UniversityPhysik-Institut, University of ZürichLIBPhys, Department of Physics, University of CoimbraNew York University Abu Dhabi, Center for Astro, Particle and Planetary PhysicsDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaMax-Planck-Institut für KernphysikInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterPhysikalisches Institut, Universität FreiburgLPNHE, Sorbonne Université, CNRS/IN2P3Department of Physics and Astronomy, University of Bologna and INFN-BolognaDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzPhysics Department, Columbia UniversityDepartment of Physics, University of California San DiegoLIBPhys, Department of Physics, University of CoimbraMax-Planck-Institut für KernphysikKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoDepartment of Physics, Oskar Klein Centre, Stockholm University, AlbaNovaMax-Planck-Institut für KernphysikSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesPhysikalisches Institut, Universität FreiburgINAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-TorinoDepartment of Physics and Astronomy, Rice UniversityPhysikalisches Institut, Universität FreiburgInstitute for Astroparticle Physics, Karlsruhe Institute of TechnologyPhysik-Institut, University of ZürichInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzPhysik-Institut, University of ZürichMax-Planck-Institut für KernphysikPhysics Department, Columbia UniversityPhysics Department, Columbia UniversityKamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of TokyoDepartment of Physics, University of California San DiegoPhysics Department, Columbia UniversityDepartment of Physics, Kavli Institute for Cosmological Physics, University of ChicagoDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaPhysics Department, Columbia UniversityDepartment of Physics, University of California San DiegoPhysics Department, Columbia UniversityForschungsreaktor TRIGA Mainz, Johannes Gutenberg-Universität MainzForschungsreaktor TRIGA Mainz, Johannes Gutenberg-Universität MainzAbstract 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.https://doi.org/10.1140/epjc/s10052-023-11512-z |
| spellingShingle | 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 Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source European Physical Journal C: Particles and Fields |
| title | Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source |
| title_full | Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source |
| title_fullStr | Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source |
| title_full_unstemmed | Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source |
| title_short | Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$ 37 Ar source |
| title_sort | low energy calibration of xenon1t with an internal textbf 37 37 ar source |
| url | https://doi.org/10.1140/epjc/s10052-023-11512-z |
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lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jconrad lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jjcuencagarcia lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jpcussonneau lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT vdandrea lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mpdecowski lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pdigangi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sdipede lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sdiglio lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT keitel lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT aelykov lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sfarrell lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT adferella lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cferrari lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT hfischer lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT wfulgione lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pgaemers lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT rgaior lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT agallorosso lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mgalloway lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT fgao lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT rgladebeucke lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lgrandi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jgrigat lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mguida lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT rhammann lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ahiguera lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT chils lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lhoetzsch lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jhowlett lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT miacovacci lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT yitow lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jjakob lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT fjoerg lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ajoy lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT nkato lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mkara lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pkavrigin lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT skazama lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mkobayashi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gkoltman lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT akopec lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT fkuger lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT hlandsman lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT rflang lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT llevinson lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ili lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sli lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sliang lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT slindemann lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mlindner lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kliu lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jloizeau lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT flombardi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jlong lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jamlopes lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT yma lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cmacolino lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jmahlstedt lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT amancuso lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lmanenti lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT fmarignetti lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT tmarrodanundagoitia lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kmartens lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jmasbou lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dmasson lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT emasson lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT smastroianni lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mmessina lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kmiuchi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kmizukoshi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT amolinario lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT smoriyama lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kmora lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ymosbacher lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mmurra lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jmuller lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kni lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT uoberlack lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT bpaetsch lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jpalacio lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT rperes lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cpeters lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jpienaar lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mpierre lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT vpizzella lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gplante lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jqi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jqin lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dramirezgarcia lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sreichard lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT arocchetti lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT nrupp lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lsanchez lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT psanchezlucas lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jmfdossantos lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT isarnoff lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gsartorelli lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jschreiner lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dschulte lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pschulte lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT hschulzeeißing lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mschumann lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lscottolavina lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mselvi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT fsemeria lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pshagin lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT sshi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT eshockley lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT msilva lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT hsimgen lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT atakeda lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT pltan lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT aterliuk lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dthers lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ftoschi lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gtrinchero lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ctunnell lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT ftonnies lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT kvalerius lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gvolta lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cweinheimer lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mweiss lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dwenz lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cwittweg lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT twolf lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT dxu lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT zxu lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT myamashita lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lyang lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jye lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT lyuan lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT gzavattini lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT szerbo lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT mzhong lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT tzhu lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT cgeppert lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT jriemer lowenergycalibrationofxenon1twithaninternaltextbf3737arsource AT xenoncollaboration lowenergycalibrationofxenon1twithaninternaltextbf3737arsource |