Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory
- Autores
- Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, Ingomar; Almela, A.; Alvarez Muñiz, J.; Alves Batista, R.; Anastasi, G. A.; Anchordoqui, Luis A.; Andrada, Betiana Eugenia; Andringa, S.; Aramo, C.; Araújo Ferreira, P. R.; Asorey, H.; Assis, P.; Avila, G.; Badescu, A. M.; Bakalova, A.; Balaceanu, A.; Barbato, F.; Barreira Luz, R. J.; Becker, K. H.; Bellido, J. A.; Berat, C.; Bertaina, M. E.; Bertou, Xavier Pierre Louis; Biermann, P. L.; Bister, T.; Gollan Scilipotti, Fernando Daniel
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the muon content of extensive air showers (EAS). It consists of an array of 61 water Cherenkov detectors on a denser spacing in combination with underground scintillation detectors used for muon density measurement. Each detector is composed of three scintillation modules, with 10 m2 detection area per module, buried at 2.3 m depth, resulting in a total detection area of 30 m2 . Silicon photomultiplier sensors (SiPM) measure the amount of scintillation light generated by charged particles traversing the modules. In this paper, the design of the front-end electronics to process the signals of those SiPMs and test results from the laboratory and from the Pierre Auger Observatory are described. Compared to our previous prototype, the new electronics shows a higher performance, higher efficiency and lower power consumption, and it has a new acquisition system with increased dynamic range that allows measurements closer to the shower core. The new acquisition system is based on the measurement of the total charge signal that the muonic component of the cosmic ray shower generates in the detector.
Fil: Aab, A.. Radboud Universiteit Nijmegen; Países Bajos
Fil: Abreu, P.. Instituto Superior Tecnico; Portugal
Fil: Aglietta, M.. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Albury, J. M.. University of Adelaide; Australia
Fil: Allekotte, Ingomar. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Almela, A.. Universidad Nacional de San Martín; Argentina. Universidad Tecnológica Nacional; Argentina
Fil: Alvarez Muñiz, J.. Universidad de Santiago de Compostela; España
Fil: Alves Batista, R.. Radboud Universiteit Nijmegen; Países Bajos
Fil: Anastasi, G. A.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Anchordoqui, Luis A.. City University of New York; Estados Unidos
Fil: Andrada, Betiana Eugenia. Universidad Nacional de San Martín; Argentina
Fil: Andringa, S.. Instituto Superior Tecnico; Portugal
Fil: Aramo, C.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Araújo Ferreira, P. R.. Rwth Aachen University; Alemania
Fil: Asorey, H.. Universidad Nacional de San Martín; Argentina
Fil: Assis, P.. Instituto Superior Tecnico; Portugal
Fil: Avila, G.. Observatorio Pierre Auger; Argentina
Fil: Badescu, A. M.. University Politehnica Of Bucharest; Rumania
Fil: Bakalova, A.. The Czech Academy Of Sciences; República Checa
Fil: Balaceanu, A.. “Horia Hulubei” National Institute for Physics and Nuclear Engineering, Bucharest-Magurele; Rumania
Fil: Barbato, F.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Barreira Luz, R. J.. Instituto Superior Tecnico; Portugal
Fil: Becker, K. H.. Bergische Universität Wuppertal; Alemania
Fil: Bellido, J. A.. University of Adelaide; Australia
Fil: Berat, C.. Universite Grenoble Alpes; Francia
Fil: Bertaina, M. E.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Bertou, Xavier Pierre Louis. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Biermann, P. L.. Max Planck Institute For Radio Astronomy; Alemania
Fil: Bister, T.. Rwth Aachen University; Alemania
Fil: Gollan Scilipotti, Fernando Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Instituto de Tecnología en Detección y Astropartículas. Comisión Nacional de Energía Atómica. Instituto de Tecnología en Detección y Astropartículas. Universidad Nacional de San Martín. Instituto de Tecnología en Detección y Astropartículas; Argentina - Materia
-
APDS
CALIBRATION AND FITTING METHODS; PERFORMANCE OF HIGH ENERGY PHYSICS DETECTORS; PHOTON DETECTORS FOR UV
CCDS
CLUSTER FINDING
CMOS IMAGERS
EBCCDS
EMCCDS
ETC)
FRONT-END ELECTRONICS FOR DETECTOR READOUT; PATTERN RECOGNITION
G-APDS
SI-PMTS
VISIBLE AND IR PHOTONS (SOLID-STATE) (PIN DIODES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/182627
Ver los metadatos del registro completo
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Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger ObservatoryAab, A.Abreu, P.Aglietta, M.Albury, J. M.Allekotte, IngomarAlmela, A.Alvarez Muñiz, J.Alves Batista, R.Anastasi, G. A.Anchordoqui, Luis A.Andrada, Betiana EugeniaAndringa, S.Aramo, C.Araújo Ferreira, P. R.Asorey, H.Assis, P.Avila, G.Badescu, A. M.Bakalova, A.Balaceanu, A.Barbato, F.Barreira Luz, R. J.Becker, K. H.Bellido, J. A.Berat, C.Bertaina, M. E.Bertou, Xavier Pierre LouisBiermann, P. L.Bister, T.Gollan Scilipotti, Fernando DanielAPDSCALIBRATION AND FITTING METHODS; PERFORMANCE OF HIGH ENERGY PHYSICS DETECTORS; PHOTON DETECTORS FOR UVCCDSCLUSTER FINDINGCMOS IMAGERSEBCCDSEMCCDSETC)FRONT-END ELECTRONICS FOR DETECTOR READOUT; PATTERN RECOGNITIONG-APDSSI-PMTSVISIBLE AND IR PHOTONS (SOLID-STATE) (PIN DIODEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the muon content of extensive air showers (EAS). It consists of an array of 61 water Cherenkov detectors on a denser spacing in combination with underground scintillation detectors used for muon density measurement. Each detector is composed of three scintillation modules, with 10 m2 detection area per module, buried at 2.3 m depth, resulting in a total detection area of 30 m2 . Silicon photomultiplier sensors (SiPM) measure the amount of scintillation light generated by charged particles traversing the modules. In this paper, the design of the front-end electronics to process the signals of those SiPMs and test results from the laboratory and from the Pierre Auger Observatory are described. Compared to our previous prototype, the new electronics shows a higher performance, higher efficiency and lower power consumption, and it has a new acquisition system with increased dynamic range that allows measurements closer to the shower core. The new acquisition system is based on the measurement of the total charge signal that the muonic component of the cosmic ray shower generates in the detector.Fil: Aab, A.. Radboud Universiteit Nijmegen; Países BajosFil: Abreu, P.. Instituto Superior Tecnico; PortugalFil: Aglietta, M.. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Albury, J. M.. University of Adelaide; AustraliaFil: Allekotte, Ingomar. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; ArgentinaFil: Almela, A.. Universidad Nacional de San Martín; Argentina. Universidad Tecnológica Nacional; ArgentinaFil: Alvarez Muñiz, J.. Universidad de Santiago de Compostela; EspañaFil: Alves Batista, R.. Radboud Universiteit Nijmegen; Países BajosFil: Anastasi, G. A.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Anchordoqui, Luis A.. City University of New York; Estados UnidosFil: Andrada, Betiana Eugenia. Universidad Nacional de San Martín; ArgentinaFil: Andringa, S.. Instituto Superior Tecnico; PortugalFil: Aramo, C.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Araújo Ferreira, P. R.. Rwth Aachen University; AlemaniaFil: Asorey, H.. Universidad Nacional de San Martín; ArgentinaFil: Assis, P.. Instituto Superior Tecnico; PortugalFil: Avila, G.. Observatorio Pierre Auger; ArgentinaFil: Badescu, A. M.. University Politehnica Of Bucharest; RumaniaFil: Bakalova, A.. The Czech Academy Of Sciences; República ChecaFil: Balaceanu, A.. “Horia Hulubei” National Institute for Physics and Nuclear Engineering, Bucharest-Magurele; RumaniaFil: Barbato, F.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Barreira Luz, R. J.. Instituto Superior Tecnico; PortugalFil: Becker, K. H.. Bergische Universität Wuppertal; AlemaniaFil: Bellido, J. A.. University of Adelaide; AustraliaFil: Berat, C.. Universite Grenoble Alpes; FranciaFil: Bertaina, M. E.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Bertou, Xavier Pierre Louis. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; ArgentinaFil: Biermann, P. L.. Max Planck Institute For Radio Astronomy; AlemaniaFil: Bister, T.. Rwth Aachen University; AlemaniaFil: Gollan Scilipotti, Fernando Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Instituto de Tecnología en Detección y Astropartículas. Comisión Nacional de Energía Atómica. Instituto de Tecnología en Detección y Astropartículas. Universidad Nacional de San Martín. Instituto de Tecnología en Detección y Astropartículas; ArgentinaIOP Publishing2021-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/182627Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, Ingomar; et al.; Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory; IOP Publishing; Journal of Instrumentation; 16; 1; 1-2021; 1-411748-0221CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1748-0221/16/01/P01026info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1748-0221/16/01/P01026info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:42:35Zoai:ri.conicet.gov.ar:11336/182627instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:42:36.15CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| title |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| spellingShingle |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory Aab, A. APDS CALIBRATION AND FITTING METHODS; PERFORMANCE OF HIGH ENERGY PHYSICS DETECTORS; PHOTON DETECTORS FOR UV CCDS CLUSTER FINDING CMOS IMAGERS EBCCDS EMCCDS ETC) FRONT-END ELECTRONICS FOR DETECTOR READOUT; PATTERN RECOGNITION G-APDS SI-PMTS VISIBLE AND IR PHOTONS (SOLID-STATE) (PIN DIODES |
| title_short |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| title_full |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| title_fullStr |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| title_full_unstemmed |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| title_sort |
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory |
| dc.creator.none.fl_str_mv |
Aab, A. Abreu, P. Aglietta, M. Albury, J. M. Allekotte, Ingomar Almela, A. Alvarez Muñiz, J. Alves Batista, R. Anastasi, G. A. Anchordoqui, Luis A. Andrada, Betiana Eugenia Andringa, S. Aramo, C. Araújo Ferreira, P. R. Asorey, H. Assis, P. Avila, G. Badescu, A. M. Bakalova, A. Balaceanu, A. Barbato, F. Barreira Luz, R. J. Becker, K. H. Bellido, J. A. Berat, C. Bertaina, M. E. Bertou, Xavier Pierre Louis Biermann, P. L. Bister, T. Gollan Scilipotti, Fernando Daniel |
| author |
Aab, A. |
| author_facet |
Aab, A. Abreu, P. Aglietta, M. Albury, J. M. Allekotte, Ingomar Almela, A. Alvarez Muñiz, J. Alves Batista, R. Anastasi, G. A. Anchordoqui, Luis A. Andrada, Betiana Eugenia Andringa, S. Aramo, C. Araújo Ferreira, P. R. Asorey, H. Assis, P. Avila, G. Badescu, A. M. Bakalova, A. Balaceanu, A. Barbato, F. Barreira Luz, R. J. Becker, K. H. Bellido, J. A. Berat, C. Bertaina, M. E. Bertou, Xavier Pierre Louis Biermann, P. L. Bister, T. Gollan Scilipotti, Fernando Daniel |
| author_role |
author |
| author2 |
Abreu, P. Aglietta, M. Albury, J. M. Allekotte, Ingomar Almela, A. Alvarez Muñiz, J. Alves Batista, R. Anastasi, G. A. Anchordoqui, Luis A. Andrada, Betiana Eugenia Andringa, S. Aramo, C. Araújo Ferreira, P. R. Asorey, H. Assis, P. Avila, G. Badescu, A. M. Bakalova, A. Balaceanu, A. Barbato, F. Barreira Luz, R. J. Becker, K. H. Bellido, J. A. Berat, C. Bertaina, M. E. Bertou, Xavier Pierre Louis Biermann, P. L. Bister, T. Gollan Scilipotti, Fernando Daniel |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
APDS CALIBRATION AND FITTING METHODS; PERFORMANCE OF HIGH ENERGY PHYSICS DETECTORS; PHOTON DETECTORS FOR UV CCDS CLUSTER FINDING CMOS IMAGERS EBCCDS EMCCDS ETC) FRONT-END ELECTRONICS FOR DETECTOR READOUT; PATTERN RECOGNITION G-APDS SI-PMTS VISIBLE AND IR PHOTONS (SOLID-STATE) (PIN DIODES |
| topic |
APDS CALIBRATION AND FITTING METHODS; PERFORMANCE OF HIGH ENERGY PHYSICS DETECTORS; PHOTON DETECTORS FOR UV CCDS CLUSTER FINDING CMOS IMAGERS EBCCDS EMCCDS ETC) FRONT-END ELECTRONICS FOR DETECTOR READOUT; PATTERN RECOGNITION G-APDS SI-PMTS VISIBLE AND IR PHOTONS (SOLID-STATE) (PIN DIODES |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the muon content of extensive air showers (EAS). It consists of an array of 61 water Cherenkov detectors on a denser spacing in combination with underground scintillation detectors used for muon density measurement. Each detector is composed of three scintillation modules, with 10 m2 detection area per module, buried at 2.3 m depth, resulting in a total detection area of 30 m2 . Silicon photomultiplier sensors (SiPM) measure the amount of scintillation light generated by charged particles traversing the modules. In this paper, the design of the front-end electronics to process the signals of those SiPMs and test results from the laboratory and from the Pierre Auger Observatory are described. Compared to our previous prototype, the new electronics shows a higher performance, higher efficiency and lower power consumption, and it has a new acquisition system with increased dynamic range that allows measurements closer to the shower core. The new acquisition system is based on the measurement of the total charge signal that the muonic component of the cosmic ray shower generates in the detector. Fil: Aab, A.. Radboud Universiteit Nijmegen; Países Bajos Fil: Abreu, P.. Instituto Superior Tecnico; Portugal Fil: Aglietta, M.. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; Italia Fil: Albury, J. M.. University of Adelaide; Australia Fil: Allekotte, Ingomar. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina Fil: Almela, A.. Universidad Nacional de San Martín; Argentina. Universidad Tecnológica Nacional; Argentina Fil: Alvarez Muñiz, J.. Universidad de Santiago de Compostela; España Fil: Alves Batista, R.. Radboud Universiteit Nijmegen; Países Bajos Fil: Anastasi, G. A.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; Italia Fil: Anchordoqui, Luis A.. City University of New York; Estados Unidos Fil: Andrada, Betiana Eugenia. Universidad Nacional de San Martín; Argentina Fil: Andringa, S.. Instituto Superior Tecnico; Portugal Fil: Aramo, C.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Araújo Ferreira, P. R.. Rwth Aachen University; Alemania Fil: Asorey, H.. Universidad Nacional de San Martín; Argentina Fil: Assis, P.. Instituto Superior Tecnico; Portugal Fil: Avila, G.. Observatorio Pierre Auger; Argentina Fil: Badescu, A. M.. University Politehnica Of Bucharest; Rumania Fil: Bakalova, A.. The Czech Academy Of Sciences; República Checa Fil: Balaceanu, A.. “Horia Hulubei” National Institute for Physics and Nuclear Engineering, Bucharest-Magurele; Rumania Fil: Barbato, F.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Fisica Nucleare; Italia Fil: Barreira Luz, R. J.. Instituto Superior Tecnico; Portugal Fil: Becker, K. H.. Bergische Universität Wuppertal; Alemania Fil: Bellido, J. A.. University of Adelaide; Australia Fil: Berat, C.. Universite Grenoble Alpes; Francia Fil: Bertaina, M. E.. Università di Torino; Italia. Istituto Nazionale di Fisica Nucleare; Italia Fil: Bertou, Xavier Pierre Louis. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina Fil: Biermann, P. L.. Max Planck Institute For Radio Astronomy; Alemania Fil: Bister, T.. Rwth Aachen University; Alemania Fil: Gollan Scilipotti, Fernando Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Instituto de Tecnología en Detección y Astropartículas. Comisión Nacional de Energía Atómica. Instituto de Tecnología en Detección y Astropartículas. Universidad Nacional de San Martín. Instituto de Tecnología en Detección y Astropartículas; Argentina |
| description |
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the muon content of extensive air showers (EAS). It consists of an array of 61 water Cherenkov detectors on a denser spacing in combination with underground scintillation detectors used for muon density measurement. Each detector is composed of three scintillation modules, with 10 m2 detection area per module, buried at 2.3 m depth, resulting in a total detection area of 30 m2 . Silicon photomultiplier sensors (SiPM) measure the amount of scintillation light generated by charged particles traversing the modules. In this paper, the design of the front-end electronics to process the signals of those SiPMs and test results from the laboratory and from the Pierre Auger Observatory are described. Compared to our previous prototype, the new electronics shows a higher performance, higher efficiency and lower power consumption, and it has a new acquisition system with increased dynamic range that allows measurements closer to the shower core. The new acquisition system is based on the measurement of the total charge signal that the muonic component of the cosmic ray shower generates in the detector. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021-01 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/182627 Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, Ingomar; et al.; Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory; IOP Publishing; Journal of Instrumentation; 16; 1; 1-2021; 1-41 1748-0221 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/182627 |
| identifier_str_mv |
Aab, A.; Abreu, P.; Aglietta, M.; Albury, J. M.; Allekotte, Ingomar; et al.; Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory; IOP Publishing; Journal of Instrumentation; 16; 1; 1-2021; 1-41 1748-0221 CONICET Digital CONICET |
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eng |
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eng |
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IOP Publishing |
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IOP Publishing |
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