A high precision calibration of the nonlinear energy response at Daya Bay
A high precision calibration of the nonlinearity in the energy response of the Daya Bay Reactor Neutrino Experiment’s antineutrino detectors is presented in detail. The energy nonlinearity originates from the particle-dependent light yield of the scintillator and charge-dependent electronics respons...
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Veröffentlicht in: | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Accelerators, spectrometers, detectors and associated equipment, 2019-10, Vol.940 (C), p.230-242 |
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creator | Adey, D. An, F.P. Balantekin, A.B. Chang, Y. Chen, H.S. Chen, Y.X. Cheng, J. Chu, M.C. Chukanov, A. Cummings, J.P. Dash, N. Deng, F.S. Dove, J. Gong, G.H. Gong, H. Guo, J.Y. Guo, L. Guo, X.H. Guo, Y.H. Hackenburg, R.W. Hor, Y.K. Hsiung, Y.B. Huang, H.X. Huber, P. Jaffe, D.E. Jen, K.L. Ji, X.L. Ji, X.P. Kettell, S.H. Koerner, L.W. Kramer, M. Langford, T.J. Lee, J.H.C. Leung, J.K.C. Li, C. Li, F. Li, H.L. Li, Q.J. Li, S. Li, S.C. Li, S.J. Li, X.N. Li, X.Q. Lin, C.J. Lin, S.K. Link, J.M. Littenberg, L. Littlejohn, B.R. Liu, J.C. Ma, Y.Q. Marshall, C. McKeown, R.D. Mitchell, I. Lepin, L. Mora Napolitano, J. Naumova, E. Ochoa-Ricoux, J.P. Olshevskiy, A. Pan, H.-R. Park, J. Pec, V. Peng, J.C. Pinsky, L. Pun, C.S.J. Qi, F.Z. Qian, X. Raper, N. Ren, J. Rosero, R. Roskovec, B. Ruan, X.C. Sun, J.L. Treskov, K. Tse, W.-H. Tull, C.E. Wang, N.Y. Wang, R.G. Wang, W. Wang, X. Wang, Y. Wang, Y.F. Wei, H.Y. Wei, L.H. Wen, L.J. Wong, S.C.F. Xing, Z.Z. Xu, J.L. Xue, T. Yang, L. Yang, Y.Z. Ye, M. Young, B.L. Yu, H.Z. Zeng, Y. Zhang, C. Zhang, H.H. Zhang, Q.M. Zhang, R. Zhang, Z.P. Zhuang, H.L. |
description | A high precision calibration of the nonlinearity in the energy response of the Daya Bay Reactor Neutrino Experiment’s antineutrino detectors is presented in detail. The energy nonlinearity originates from the particle-dependent light yield of the scintillator and charge-dependent electronics response. The nonlinearity model is constrained by γ calibration points from deployed and naturally occurring radioactive sources, the β spectrum from 12B decays, and a direct measurement of the electronics nonlinearity with a new flash analog-to-digital converter readout system. Less than 0.5% uncertainty in the energy nonlinearity calibration is achieved for positrons of kinetic energies greater than 1 MeV. |
doi_str_mv | 10.1016/j.nima.2019.06.031 |
format | Article |
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Mora ; Napolitano, J. ; Naumova, E. ; Ochoa-Ricoux, J.P. ; Olshevskiy, A. ; Pan, H.-R. ; Park, J. ; Pec, V. ; Peng, J.C. ; Pinsky, L. ; Pun, C.S.J. ; Qi, F.Z. ; Qian, X. ; Raper, N. ; Ren, J. ; Rosero, R. ; Roskovec, B. ; Ruan, X.C. ; Sun, J.L. ; Treskov, K. ; Tse, W.-H. ; Tull, C.E. ; Wang, N.Y. ; Wang, R.G. ; Wang, W. ; Wang, X. ; Wang, Y. ; Wang, Y.F. ; Wei, H.Y. ; Wei, L.H. ; Wen, L.J. ; Wong, S.C.F. ; Xing, Z.Z. ; Xu, J.L. ; Xue, T. ; Yang, L. ; Yang, Y.Z. ; Ye, M. ; Young, B.L. ; Yu, H.Z. ; Zeng, Y. ; Zhang, C. ; Zhang, H.H. ; Zhang, Q.M. ; Zhang, R. ; Zhang, Z.P. ; Zhuang, H.L.</creator><creatorcontrib>Adey, D. ; An, F.P. ; Balantekin, A.B. ; Chang, Y. ; Chen, H.S. ; Chen, Y.X. ; Cheng, J. ; Chu, M.C. ; Chukanov, A. ; Cummings, J.P. ; Dash, N. ; Deng, F.S. ; Dove, J. ; Gong, G.H. ; Gong, H. ; Guo, J.Y. ; Guo, L. ; Guo, X.H. ; Guo, Y.H. ; Hackenburg, R.W. ; Hor, Y.K. ; Hsiung, Y.B. ; Huang, H.X. ; Huber, P. ; Jaffe, D.E. ; Jen, K.L. ; Ji, X.L. ; Ji, X.P. ; Kettell, S.H. ; Koerner, L.W. ; Kramer, M. ; Langford, T.J. ; Lee, J.H.C. ; Leung, J.K.C. ; Li, C. ; Li, F. ; Li, H.L. ; Li, Q.J. ; Li, S. ; Li, S.C. ; Li, S.J. ; Li, X.N. ; Li, X.Q. ; Lin, C.J. ; Lin, S.K. ; Link, J.M. ; Littenberg, L. ; Littlejohn, B.R. ; Liu, J.C. ; Ma, Y.Q. ; Marshall, C. ; McKeown, R.D. ; Mitchell, I. ; Lepin, L. Mora ; Napolitano, J. ; Naumova, E. ; Ochoa-Ricoux, J.P. ; Olshevskiy, A. ; Pan, H.-R. ; Park, J. ; Pec, V. ; Peng, J.C. ; Pinsky, L. ; Pun, C.S.J. ; Qi, F.Z. ; Qian, X. ; Raper, N. ; Ren, J. ; Rosero, R. ; Roskovec, B. ; Ruan, X.C. ; Sun, J.L. ; Treskov, K. ; Tse, W.-H. ; Tull, C.E. ; Wang, N.Y. ; Wang, R.G. ; Wang, W. ; Wang, X. ; Wang, Y. ; Wang, Y.F. ; Wei, H.Y. ; Wei, L.H. ; Wen, L.J. ; Wong, S.C.F. ; Xing, Z.Z. ; Xu, J.L. ; Xue, T. ; Yang, L. ; Yang, Y.Z. ; Ye, M. ; Young, B.L. ; Yu, H.Z. ; Zeng, Y. ; Zhang, C. ; Zhang, H.H. ; Zhang, Q.M. ; Zhang, R. ; Zhang, Z.P. ; Zhuang, H.L.</creatorcontrib><description>A high precision calibration of the nonlinearity in the energy response of the Daya Bay Reactor Neutrino Experiment’s antineutrino detectors is presented in detail. The energy nonlinearity originates from the particle-dependent light yield of the scintillator and charge-dependent electronics response. The nonlinearity model is constrained by γ calibration points from deployed and naturally occurring radioactive sources, the β spectrum from 12B decays, and a direct measurement of the electronics nonlinearity with a new flash analog-to-digital converter readout system. Less than 0.5% uncertainty in the energy nonlinearity calibration is achieved for positrons of kinetic energies greater than 1 MeV.</description><identifier>ISSN: 0168-9002</identifier><identifier>EISSN: 1872-9576</identifier><identifier>DOI: 10.1016/j.nima.2019.06.031</identifier><language>eng</language><publisher>Netherlands: Elsevier B.V</publisher><subject>Daya Bay ; Energy calibration ; Liquid scintillator ; Neutrino</subject><ispartof>Nuclear instruments & methods in physics research. 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Mora</creatorcontrib><creatorcontrib>Napolitano, J.</creatorcontrib><creatorcontrib>Naumova, E.</creatorcontrib><creatorcontrib>Ochoa-Ricoux, J.P.</creatorcontrib><creatorcontrib>Olshevskiy, A.</creatorcontrib><creatorcontrib>Pan, H.-R.</creatorcontrib><creatorcontrib>Park, J.</creatorcontrib><creatorcontrib>Pec, V.</creatorcontrib><creatorcontrib>Peng, J.C.</creatorcontrib><creatorcontrib>Pinsky, L.</creatorcontrib><creatorcontrib>Pun, C.S.J.</creatorcontrib><creatorcontrib>Qi, F.Z.</creatorcontrib><creatorcontrib>Qian, X.</creatorcontrib><creatorcontrib>Raper, N.</creatorcontrib><creatorcontrib>Ren, J.</creatorcontrib><creatorcontrib>Rosero, R.</creatorcontrib><creatorcontrib>Roskovec, B.</creatorcontrib><creatorcontrib>Ruan, X.C.</creatorcontrib><creatorcontrib>Sun, J.L.</creatorcontrib><creatorcontrib>Treskov, K.</creatorcontrib><creatorcontrib>Tse, W.-H.</creatorcontrib><creatorcontrib>Tull, C.E.</creatorcontrib><creatorcontrib>Wang, N.Y.</creatorcontrib><creatorcontrib>Wang, R.G.</creatorcontrib><creatorcontrib>Wang, W.</creatorcontrib><creatorcontrib>Wang, X.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Wang, Y.F.</creatorcontrib><creatorcontrib>Wei, H.Y.</creatorcontrib><creatorcontrib>Wei, L.H.</creatorcontrib><creatorcontrib>Wen, L.J.</creatorcontrib><creatorcontrib>Wong, S.C.F.</creatorcontrib><creatorcontrib>Xing, Z.Z.</creatorcontrib><creatorcontrib>Xu, J.L.</creatorcontrib><creatorcontrib>Xue, T.</creatorcontrib><creatorcontrib>Yang, L.</creatorcontrib><creatorcontrib>Yang, Y.Z.</creatorcontrib><creatorcontrib>Ye, M.</creatorcontrib><creatorcontrib>Young, B.L.</creatorcontrib><creatorcontrib>Yu, H.Z.</creatorcontrib><creatorcontrib>Zeng, Y.</creatorcontrib><creatorcontrib>Zhang, C.</creatorcontrib><creatorcontrib>Zhang, H.H.</creatorcontrib><creatorcontrib>Zhang, Q.M.</creatorcontrib><creatorcontrib>Zhang, R.</creatorcontrib><creatorcontrib>Zhang, Z.P.</creatorcontrib><creatorcontrib>Zhuang, H.L.</creatorcontrib><title>A high precision calibration of the nonlinear energy response at Daya Bay</title><title>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</title><description>A high precision calibration of the nonlinearity in the energy response of the Daya Bay Reactor Neutrino Experiment’s antineutrino detectors is presented in detail. The energy nonlinearity originates from the particle-dependent light yield of the scintillator and charge-dependent electronics response. The nonlinearity model is constrained by γ calibration points from deployed and naturally occurring radioactive sources, the β spectrum from 12B decays, and a direct measurement of the electronics nonlinearity with a new flash analog-to-digital converter readout system. Less than 0.5% uncertainty in the energy nonlinearity calibration is achieved for positrons of kinetic energies greater than 1 MeV.</description><subject>Daya Bay</subject><subject>Energy calibration</subject><subject>Liquid scintillator</subject><subject>Neutrino</subject><issn>0168-9002</issn><issn>1872-9576</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWKt_wFPwvms-uskueKnfhYIXPYdsdtJNqUlJgrD_3iz17FxmDs_7MjwI3VJSU0LF_b727lvXjNCuJqImnJ6hBW0lq7pGinO0KFBbdYSwS3SV0p6U6WS7QJs1Ht1uxMcIxiUXPDb64Pqo83wHi_MI2Ad_cB50xOAh7iYcIR2DT4B1xs960vhRT9fowupDgpu_vURfry-fT-_V9uNt87TeVoZLmisLwJg1vWBy4NrYvuVUSNp2hDWDNL2VLbGatExLI7VsrBVS9pxqa3tgqxVfortTb0jZqWRcBjOa4D2YrGjDOsFlgdgJMjGkFMGqYyyC4qQoUbMxtVezMTUbU0SoYqyEHk4hKO__OIhzO3gDg4tz-RDcf_Ffusp0ww</recordid><startdate>20191001</startdate><enddate>20191001</enddate><creator>Adey, D.</creator><creator>An, F.P.</creator><creator>Balantekin, A.B.</creator><creator>Chang, Y.</creator><creator>Chen, H.S.</creator><creator>Chen, Y.X.</creator><creator>Cheng, J.</creator><creator>Chu, M.C.</creator><creator>Chukanov, A.</creator><creator>Cummings, J.P.</creator><creator>Dash, N.</creator><creator>Deng, F.S.</creator><creator>Dove, J.</creator><creator>Gong, G.H.</creator><creator>Gong, H.</creator><creator>Guo, J.Y.</creator><creator>Guo, L.</creator><creator>Guo, X.H.</creator><creator>Guo, Y.H.</creator><creator>Hackenburg, R.W.</creator><creator>Hor, Y.K.</creator><creator>Hsiung, Y.B.</creator><creator>Huang, H.X.</creator><creator>Huber, P.</creator><creator>Jaffe, D.E.</creator><creator>Jen, K.L.</creator><creator>Ji, X.L.</creator><creator>Ji, X.P.</creator><creator>Kettell, S.H.</creator><creator>Koerner, L.W.</creator><creator>Kramer, M.</creator><creator>Langford, T.J.</creator><creator>Lee, J.H.C.</creator><creator>Leung, J.K.C.</creator><creator>Li, C.</creator><creator>Li, F.</creator><creator>Li, H.L.</creator><creator>Li, Q.J.</creator><creator>Li, S.</creator><creator>Li, S.C.</creator><creator>Li, S.J.</creator><creator>Li, X.N.</creator><creator>Li, X.Q.</creator><creator>Lin, C.J.</creator><creator>Lin, S.K.</creator><creator>Link, J.M.</creator><creator>Littenberg, L.</creator><creator>Littlejohn, B.R.</creator><creator>Liu, J.C.</creator><creator>Ma, Y.Q.</creator><creator>Marshall, C.</creator><creator>McKeown, R.D.</creator><creator>Mitchell, I.</creator><creator>Lepin, L. Mora</creator><creator>Napolitano, J.</creator><creator>Naumova, E.</creator><creator>Ochoa-Ricoux, J.P.</creator><creator>Olshevskiy, A.</creator><creator>Pan, H.-R.</creator><creator>Park, J.</creator><creator>Pec, V.</creator><creator>Peng, J.C.</creator><creator>Pinsky, L.</creator><creator>Pun, C.S.J.</creator><creator>Qi, F.Z.</creator><creator>Qian, X.</creator><creator>Raper, N.</creator><creator>Ren, J.</creator><creator>Rosero, R.</creator><creator>Roskovec, B.</creator><creator>Ruan, X.C.</creator><creator>Sun, J.L.</creator><creator>Treskov, K.</creator><creator>Tse, W.-H.</creator><creator>Tull, C.E.</creator><creator>Wang, N.Y.</creator><creator>Wang, R.G.</creator><creator>Wang, W.</creator><creator>Wang, X.</creator><creator>Wang, Y.</creator><creator>Wang, Y.F.</creator><creator>Wei, H.Y.</creator><creator>Wei, L.H.</creator><creator>Wen, L.J.</creator><creator>Wong, S.C.F.</creator><creator>Xing, Z.Z.</creator><creator>Xu, J.L.</creator><creator>Xue, T.</creator><creator>Yang, L.</creator><creator>Yang, Y.Z.</creator><creator>Ye, M.</creator><creator>Young, B.L.</creator><creator>Yu, H.Z.</creator><creator>Zeng, Y.</creator><creator>Zhang, C.</creator><creator>Zhang, H.H.</creator><creator>Zhang, Q.M.</creator><creator>Zhang, R.</creator><creator>Zhang, Z.P.</creator><creator>Zhuang, H.L.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20191001</creationdate><title>A high precision calibration of the nonlinear energy response at Daya Bay</title><author>Adey, D. ; An, F.P. ; Balantekin, A.B. ; Chang, Y. ; Chen, H.S. ; Chen, Y.X. ; Cheng, J. ; Chu, M.C. ; Chukanov, A. ; Cummings, J.P. ; Dash, N. ; Deng, F.S. ; Dove, J. ; Gong, G.H. ; Gong, H. ; Guo, J.Y. ; Guo, L. ; Guo, X.H. ; Guo, Y.H. ; Hackenburg, R.W. ; Hor, Y.K. ; Hsiung, Y.B. ; Huang, H.X. ; Huber, P. ; Jaffe, D.E. ; Jen, K.L. ; Ji, X.L. ; Ji, X.P. ; Kettell, S.H. ; Koerner, L.W. ; Kramer, M. ; Langford, T.J. ; Lee, J.H.C. ; Leung, J.K.C. ; Li, C. ; Li, F. ; Li, H.L. ; Li, Q.J. ; Li, S. ; Li, S.C. ; Li, S.J. ; Li, X.N. ; Li, X.Q. ; Lin, C.J. ; Lin, S.K. ; Link, J.M. ; Littenberg, L. ; Littlejohn, B.R. ; Liu, J.C. ; Ma, Y.Q. ; Marshall, C. ; McKeown, R.D. ; Mitchell, I. ; Lepin, L. Mora ; Napolitano, J. ; Naumova, E. ; Ochoa-Ricoux, J.P. ; Olshevskiy, A. ; Pan, H.-R. ; Park, J. ; Pec, V. ; Peng, J.C. ; Pinsky, L. ; Pun, C.S.J. ; Qi, F.Z. ; Qian, X. ; Raper, N. ; Ren, J. ; Rosero, R. ; Roskovec, B. ; Ruan, X.C. ; Sun, J.L. ; Treskov, K. ; Tse, W.-H. ; Tull, C.E. ; Wang, N.Y. ; Wang, R.G. ; Wang, W. ; Wang, X. ; Wang, Y. ; Wang, Y.F. ; Wei, H.Y. ; Wei, L.H. ; Wen, L.J. ; Wong, S.C.F. ; Xing, Z.Z. ; Xu, J.L. ; Xue, T. ; Yang, L. ; Yang, Y.Z. ; Ye, M. ; Young, B.L. ; Yu, H.Z. ; Zeng, Y. ; Zhang, C. ; Zhang, H.H. ; Zhang, Q.M. ; Zhang, R. ; Zhang, Z.P. ; Zhuang, H.L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c371t-fee22fcb627d3acfb83167189025d7cbf780fa082a7c7a75ff677b31affbe2443</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Daya Bay</topic><topic>Energy calibration</topic><topic>Liquid scintillator</topic><topic>Neutrino</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Adey, D.</creatorcontrib><creatorcontrib>An, F.P.</creatorcontrib><creatorcontrib>Balantekin, A.B.</creatorcontrib><creatorcontrib>Chang, Y.</creatorcontrib><creatorcontrib>Chen, H.S.</creatorcontrib><creatorcontrib>Chen, Y.X.</creatorcontrib><creatorcontrib>Cheng, J.</creatorcontrib><creatorcontrib>Chu, M.C.</creatorcontrib><creatorcontrib>Chukanov, A.</creatorcontrib><creatorcontrib>Cummings, J.P.</creatorcontrib><creatorcontrib>Dash, N.</creatorcontrib><creatorcontrib>Deng, F.S.</creatorcontrib><creatorcontrib>Dove, J.</creatorcontrib><creatorcontrib>Gong, G.H.</creatorcontrib><creatorcontrib>Gong, H.</creatorcontrib><creatorcontrib>Guo, J.Y.</creatorcontrib><creatorcontrib>Guo, L.</creatorcontrib><creatorcontrib>Guo, X.H.</creatorcontrib><creatorcontrib>Guo, Y.H.</creatorcontrib><creatorcontrib>Hackenburg, R.W.</creatorcontrib><creatorcontrib>Hor, Y.K.</creatorcontrib><creatorcontrib>Hsiung, Y.B.</creatorcontrib><creatorcontrib>Huang, H.X.</creatorcontrib><creatorcontrib>Huber, P.</creatorcontrib><creatorcontrib>Jaffe, D.E.</creatorcontrib><creatorcontrib>Jen, K.L.</creatorcontrib><creatorcontrib>Ji, X.L.</creatorcontrib><creatorcontrib>Ji, X.P.</creatorcontrib><creatorcontrib>Kettell, S.H.</creatorcontrib><creatorcontrib>Koerner, L.W.</creatorcontrib><creatorcontrib>Kramer, M.</creatorcontrib><creatorcontrib>Langford, T.J.</creatorcontrib><creatorcontrib>Lee, J.H.C.</creatorcontrib><creatorcontrib>Leung, J.K.C.</creatorcontrib><creatorcontrib>Li, C.</creatorcontrib><creatorcontrib>Li, F.</creatorcontrib><creatorcontrib>Li, H.L.</creatorcontrib><creatorcontrib>Li, Q.J.</creatorcontrib><creatorcontrib>Li, S.</creatorcontrib><creatorcontrib>Li, S.C.</creatorcontrib><creatorcontrib>Li, S.J.</creatorcontrib><creatorcontrib>Li, X.N.</creatorcontrib><creatorcontrib>Li, X.Q.</creatorcontrib><creatorcontrib>Lin, C.J.</creatorcontrib><creatorcontrib>Lin, S.K.</creatorcontrib><creatorcontrib>Link, J.M.</creatorcontrib><creatorcontrib>Littenberg, L.</creatorcontrib><creatorcontrib>Littlejohn, B.R.</creatorcontrib><creatorcontrib>Liu, J.C.</creatorcontrib><creatorcontrib>Ma, Y.Q.</creatorcontrib><creatorcontrib>Marshall, C.</creatorcontrib><creatorcontrib>McKeown, R.D.</creatorcontrib><creatorcontrib>Mitchell, I.</creatorcontrib><creatorcontrib>Lepin, L. Mora</creatorcontrib><creatorcontrib>Napolitano, J.</creatorcontrib><creatorcontrib>Naumova, E.</creatorcontrib><creatorcontrib>Ochoa-Ricoux, J.P.</creatorcontrib><creatorcontrib>Olshevskiy, A.</creatorcontrib><creatorcontrib>Pan, H.-R.</creatorcontrib><creatorcontrib>Park, J.</creatorcontrib><creatorcontrib>Pec, V.</creatorcontrib><creatorcontrib>Peng, J.C.</creatorcontrib><creatorcontrib>Pinsky, L.</creatorcontrib><creatorcontrib>Pun, C.S.J.</creatorcontrib><creatorcontrib>Qi, F.Z.</creatorcontrib><creatorcontrib>Qian, X.</creatorcontrib><creatorcontrib>Raper, N.</creatorcontrib><creatorcontrib>Ren, J.</creatorcontrib><creatorcontrib>Rosero, R.</creatorcontrib><creatorcontrib>Roskovec, B.</creatorcontrib><creatorcontrib>Ruan, X.C.</creatorcontrib><creatorcontrib>Sun, J.L.</creatorcontrib><creatorcontrib>Treskov, K.</creatorcontrib><creatorcontrib>Tse, W.-H.</creatorcontrib><creatorcontrib>Tull, C.E.</creatorcontrib><creatorcontrib>Wang, N.Y.</creatorcontrib><creatorcontrib>Wang, R.G.</creatorcontrib><creatorcontrib>Wang, W.</creatorcontrib><creatorcontrib>Wang, X.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Wang, Y.F.</creatorcontrib><creatorcontrib>Wei, H.Y.</creatorcontrib><creatorcontrib>Wei, L.H.</creatorcontrib><creatorcontrib>Wen, L.J.</creatorcontrib><creatorcontrib>Wong, S.C.F.</creatorcontrib><creatorcontrib>Xing, Z.Z.</creatorcontrib><creatorcontrib>Xu, J.L.</creatorcontrib><creatorcontrib>Xue, T.</creatorcontrib><creatorcontrib>Yang, L.</creatorcontrib><creatorcontrib>Yang, Y.Z.</creatorcontrib><creatorcontrib>Ye, M.</creatorcontrib><creatorcontrib>Young, B.L.</creatorcontrib><creatorcontrib>Yu, H.Z.</creatorcontrib><creatorcontrib>Zeng, Y.</creatorcontrib><creatorcontrib>Zhang, C.</creatorcontrib><creatorcontrib>Zhang, H.H.</creatorcontrib><creatorcontrib>Zhang, Q.M.</creatorcontrib><creatorcontrib>Zhang, R.</creatorcontrib><creatorcontrib>Zhang, Z.P.</creatorcontrib><creatorcontrib>Zhuang, H.L.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adey, D.</au><au>An, F.P.</au><au>Balantekin, A.B.</au><au>Chang, Y.</au><au>Chen, H.S.</au><au>Chen, Y.X.</au><au>Cheng, J.</au><au>Chu, M.C.</au><au>Chukanov, A.</au><au>Cummings, J.P.</au><au>Dash, N.</au><au>Deng, F.S.</au><au>Dove, J.</au><au>Gong, G.H.</au><au>Gong, H.</au><au>Guo, J.Y.</au><au>Guo, L.</au><au>Guo, X.H.</au><au>Guo, Y.H.</au><au>Hackenburg, R.W.</au><au>Hor, Y.K.</au><au>Hsiung, Y.B.</au><au>Huang, H.X.</au><au>Huber, P.</au><au>Jaffe, D.E.</au><au>Jen, K.L.</au><au>Ji, X.L.</au><au>Ji, X.P.</au><au>Kettell, S.H.</au><au>Koerner, L.W.</au><au>Kramer, M.</au><au>Langford, T.J.</au><au>Lee, J.H.C.</au><au>Leung, J.K.C.</au><au>Li, C.</au><au>Li, F.</au><au>Li, H.L.</au><au>Li, Q.J.</au><au>Li, S.</au><au>Li, S.C.</au><au>Li, S.J.</au><au>Li, X.N.</au><au>Li, X.Q.</au><au>Lin, C.J.</au><au>Lin, S.K.</au><au>Link, J.M.</au><au>Littenberg, L.</au><au>Littlejohn, B.R.</au><au>Liu, J.C.</au><au>Ma, Y.Q.</au><au>Marshall, C.</au><au>McKeown, R.D.</au><au>Mitchell, I.</au><au>Lepin, L. Mora</au><au>Napolitano, J.</au><au>Naumova, E.</au><au>Ochoa-Ricoux, J.P.</au><au>Olshevskiy, A.</au><au>Pan, H.-R.</au><au>Park, J.</au><au>Pec, V.</au><au>Peng, J.C.</au><au>Pinsky, L.</au><au>Pun, C.S.J.</au><au>Qi, F.Z.</au><au>Qian, X.</au><au>Raper, N.</au><au>Ren, J.</au><au>Rosero, R.</au><au>Roskovec, B.</au><au>Ruan, X.C.</au><au>Sun, J.L.</au><au>Treskov, K.</au><au>Tse, W.-H.</au><au>Tull, C.E.</au><au>Wang, N.Y.</au><au>Wang, R.G.</au><au>Wang, W.</au><au>Wang, X.</au><au>Wang, Y.</au><au>Wang, Y.F.</au><au>Wei, H.Y.</au><au>Wei, L.H.</au><au>Wen, L.J.</au><au>Wong, S.C.F.</au><au>Xing, Z.Z.</au><au>Xu, J.L.</au><au>Xue, T.</au><au>Yang, L.</au><au>Yang, Y.Z.</au><au>Ye, M.</au><au>Young, B.L.</au><au>Yu, H.Z.</au><au>Zeng, Y.</au><au>Zhang, C.</au><au>Zhang, H.H.</au><au>Zhang, Q.M.</au><au>Zhang, R.</au><au>Zhang, Z.P.</au><au>Zhuang, H.L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A high precision calibration of the nonlinear energy response at Daya Bay</atitle><jtitle>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</jtitle><date>2019-10-01</date><risdate>2019</risdate><volume>940</volume><issue>C</issue><spage>230</spage><epage>242</epage><pages>230-242</pages><issn>0168-9002</issn><eissn>1872-9576</eissn><abstract>A high precision calibration of the nonlinearity in the energy response of the Daya Bay Reactor Neutrino Experiment’s antineutrino detectors is presented in detail. The energy nonlinearity originates from the particle-dependent light yield of the scintillator and charge-dependent electronics response. The nonlinearity model is constrained by γ calibration points from deployed and naturally occurring radioactive sources, the β spectrum from 12B decays, and a direct measurement of the electronics nonlinearity with a new flash analog-to-digital converter readout system. Less than 0.5% uncertainty in the energy nonlinearity calibration is achieved for positrons of kinetic energies greater than 1 MeV.</abstract><cop>Netherlands</cop><pub>Elsevier B.V</pub><doi>10.1016/j.nima.2019.06.031</doi><tpages>13</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0168-9002 |
ispartof | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 2019-10, Vol.940 (C), p.230-242 |
issn | 0168-9002 1872-9576 |
language | eng |
recordid | cdi_osti_scitechconnect_1529637 |
source | Elsevier ScienceDirect Journals |
subjects | Daya Bay Energy calibration Liquid scintillator Neutrino |
title | A high precision calibration of the nonlinear energy response at Daya Bay |
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