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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
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
Hauptverfasser: 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.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 242
container_issue C
container_start_page 230
container_title Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment
container_volume 940
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
fullrecord <record><control><sourceid>elsevier_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1529637</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S016890021930871X</els_id><sourcerecordid>S016890021930871X</sourcerecordid><originalsourceid>FETCH-LOGICAL-c371t-fee22fcb627d3acfb83167189025d7cbf780fa082a7c7a75ff677b31affbe2443</originalsourceid><addsrcrecordid>eNp9kE1LAzEQhoMoWKt_wFPwvms-uskueKnfhYIXPYdsdtJNqUlJgrD_3iz17FxmDs_7MjwI3VJSU0LF_b727lvXjNCuJqImnJ6hBW0lq7pGinO0KFBbdYSwS3SV0p6U6WS7QJs1Ht1uxMcIxiUXPDb64Pqo83wHi_MI2Ad_cB50xOAh7iYcIR2DT4B1xs960vhRT9fowupDgpu_vURfry-fT-_V9uNt87TeVoZLmisLwJg1vWBy4NrYvuVUSNp2hDWDNL2VLbGatExLI7VsrBVS9pxqa3tgqxVfortTb0jZqWRcBjOa4D2YrGjDOsFlgdgJMjGkFMGqYyyC4qQoUbMxtVezMTUbU0SoYqyEHk4hKO__OIhzO3gDg4tz-RDcf_Ffusp0ww</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>A high precision calibration of the nonlinear energy response at Daya Bay</title><source>Elsevier ScienceDirect Journals</source><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.</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 &amp; methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 2019-10, Vol.940 (C), p.230-242</ispartof><rights>2019 Elsevier B.V.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c371t-fee22fcb627d3acfb83167189025d7cbf780fa082a7c7a75ff677b31affbe2443</citedby><cites>FETCH-LOGICAL-c371t-fee22fcb627d3acfb83167189025d7cbf780fa082a7c7a75ff677b31affbe2443</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S016890021930871X$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,776,780,881,3537,27901,27902,65306</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/1529637$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><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><title>A high precision calibration of the nonlinear energy response at Daya Bay</title><title>Nuclear instruments &amp; 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 &amp; 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 &amp; 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
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-31T13%3A16%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20high%20precision%20calibration%20of%20the%20nonlinear%20energy%20response%20at%20Daya%20Bay&rft.jtitle=Nuclear%20instruments%20&%20methods%20in%20physics%20research.%20Section%20A,%20Accelerators,%20spectrometers,%20detectors%20and%20associated%20equipment&rft.au=Adey,%20D.&rft.date=2019-10-01&rft.volume=940&rft.issue=C&rft.spage=230&rft.epage=242&rft.pages=230-242&rft.issn=0168-9002&rft.eissn=1872-9576&rft_id=info:doi/10.1016/j.nima.2019.06.031&rft_dat=%3Celsevier_osti_%3ES016890021930871X%3C/elsevier_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_els_id=S016890021930871X&rfr_iscdi=true