Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation
The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of Y...
Ausführliche Beschreibung
Autor*in: |
Shin, B.K. [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
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2014transfer abstract |
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Umfang: |
8 |
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Übergeordnetes Werk: |
Enthalten in: The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol - Ide, C.V. ELSEVIER, 2017, a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics, Amsterdam |
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Übergeordnetes Werk: |
volume:768 ; year:2014 ; day:21 ; month:12 ; pages:96-103 ; extent:8 |
Links: |
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DOI / URN: |
10.1016/j.nima.2014.09.059 |
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Katalog-ID: |
ELV012130842 |
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520 | |a The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. | ||
520 | |a The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. | ||
650 | 7 | |a Ultra-high energy cosmic rays |2 Elsevier | |
650 | 7 | |a Air fluorescence telescope |2 Elsevier | |
650 | 7 | |a Calibration of photomultiplier |2 Elsevier | |
700 | 1 | |a Tokuno, H. |4 oth | |
700 | 1 | |a Tsunesada, Y. |4 oth | |
700 | 1 | |a Abu-Zayyad, T. |4 oth | |
700 | 1 | |a Aida, R. |4 oth | |
700 | 1 | |a Allen, M. |4 oth | |
700 | 1 | |a Anderson, R. |4 oth | |
700 | 1 | |a Azuma, R. |4 oth | |
700 | 1 | |a Barcikowski, E. |4 oth | |
700 | 1 | |a Belz, J.W. |4 oth | |
700 | 1 | |a Bergman, D.R. |4 oth | |
700 | 1 | |a Blake, S.A. |4 oth | |
700 | 1 | |a Cady, R. |4 oth | |
700 | 1 | |a Cheon, B.G. |4 oth | |
700 | 1 | |a Chiba, J. |4 oth | |
700 | 1 | |a Chikawa, M. |4 oth | |
700 | 1 | |a Cho, E.J. |4 oth | |
700 | 1 | |a Cho, W.R. |4 oth | |
700 | 1 | |a Fujii, H. |4 oth | |
700 | 1 | |a Fujii, T. |4 oth | |
700 | 1 | |a Fukuda, T. |4 oth | |
700 | 1 | |a Fukushima, M. |4 oth | |
700 | 1 | |a Hanlon, W. |4 oth | |
700 | 1 | |a Hayashi, K. |4 oth | |
700 | 1 | |a Hayashi, Y. |4 oth | |
700 | 1 | |a Hayashida, N. |4 oth | |
700 | 1 | |a Hibino, K. |4 oth | |
700 | 1 | |a Hiyama, K. |4 oth | |
700 | 1 | |a Honda, K. |4 oth | |
700 | 1 | |a Iguchi, T. |4 oth | |
700 | 1 | |a Ikeda, D. |4 oth | |
700 | 1 | |a Ikuta, K. |4 oth | |
700 | 1 | |a Inoue, N. |4 oth | |
700 | 1 | |a Ishii, T. |4 oth | |
700 | 1 | |a Ishimori, R. |4 oth | |
700 | 1 | |a Ivanov, D. |4 oth | |
700 | 1 | |a Iwamoto, S. |4 oth | |
700 | 1 | |a Jui, C.C.H. |4 oth | |
700 | 1 | |a Kadota, K. |4 oth | |
700 | 1 | |a Kakimoto, F. |4 oth | |
700 | 1 | |a Kalashev, O. |4 oth | |
700 | 1 | |a Kanbe, T. |4 oth | |
700 | 1 | |a Kasahara, K. |4 oth | |
700 | 1 | |a Kawai, H. |4 oth | |
700 | 1 | |a Kawakami, S. |4 oth | |
700 | 1 | |a Kawana, S. |4 oth | |
700 | 1 | |a Kido, E. |4 oth | |
700 | 1 | |a Kim, H.B. |4 oth | |
700 | 1 | |a Kim, H.K. |4 oth | |
700 | 1 | |a Kim, J.H. |4 oth | |
700 | 1 | |a Kim, J.H. |4 oth | |
700 | 1 | |a Kitamoto, K. |4 oth | |
700 | 1 | |a Kitamura, S. |4 oth | |
700 | 1 | |a Kitamura, Y. |4 oth | |
700 | 1 | |a Kobayashi, K. |4 oth | |
700 | 1 | |a Kobayashi, Y. |4 oth | |
700 | 1 | |a Kondo, Y. |4 oth | |
700 | 1 | |a Kuramoto, K. |4 oth | |
700 | 1 | |a Kuzmin, V. |4 oth | |
700 | 1 | |a Kwon, Y.J. |4 oth | |
700 | 1 | |a Lim, S.I. |4 oth | |
700 | 1 | |a Machida, S. |4 oth | |
700 | 1 | |a Martens, K. |4 oth | |
700 | 1 | |a Martineau, J. |4 oth | |
700 | 1 | |a Matsuda, T. |4 oth | |
700 | 1 | |a Matsuura, T. |4 oth | |
700 | 1 | |a Matsuyama, T. |4 oth | |
700 | 1 | |a Matthews, J.N. |4 oth | |
700 | 1 | |a Myers, I. |4 oth | |
700 | 1 | |a Minamino, M. |4 oth | |
700 | 1 | |a Miyata, K. |4 oth | |
700 | 1 | |a Murano, Y. |4 oth | |
700 | 1 | |a Nagasawa, K. |4 oth | |
700 | 1 | |a Nagataki, S. |4 oth | |
700 | 1 | |a Nakamura, T. |4 oth | |
700 | 1 | |a Nam, S.W. |4 oth | |
700 | 1 | |a Nonaka, T. |4 oth | |
700 | 1 | |a Ogio, S. |4 oth | |
700 | 1 | |a Ohnishi, M. |4 oth | |
700 | 1 | |a Ohoka, H. |4 oth | |
700 | 1 | |a Oki, K. |4 oth | |
700 | 1 | |a Oku, D. |4 oth | |
700 | 1 | |a Okuda, T. |4 oth | |
700 | 1 | |a Oshima, A. |4 oth | |
700 | 1 | |a Ozawa, S. |4 oth | |
700 | 1 | |a Park, I.H. |4 oth | |
700 | 1 | |a Pshirkov, M.S. |4 oth | |
700 | 1 | |a Rodriguez, D.C. |4 oth | |
700 | 1 | |a Roh, S.Y. |4 oth | |
700 | 1 | |a Rubtsov, G. |4 oth | |
700 | 1 | |a Ryu, D. |4 oth | |
700 | 1 | |a Sagawa, H. |4 oth | |
700 | 1 | |a Sakurai, N. |4 oth | |
700 | 1 | |a Sampson, A.L. |4 oth | |
700 | 1 | |a Scott, L.M. |4 oth | |
700 | 1 | |a Shah, P.D. |4 oth | |
700 | 1 | |a Shibata, F. |4 oth | |
700 | 1 | |a Shibata, T. |4 oth | |
700 | 1 | |a Shimodaira, H. |4 oth | |
700 | 1 | |a Shin, J.I. |4 oth | |
700 | 1 | |a Shirahama, T. |4 oth | |
700 | 1 | |a Smith, J.D. |4 oth | |
700 | 1 | |a Sokolsky, P. |4 oth | |
700 | 1 | |a Sonley, T.J. |4 oth | |
700 | 1 | |a Springer, R.W. |4 oth | |
700 | 1 | |a Stokes, B.T. |4 oth | |
700 | 1 | |a Stratton, S.R. |4 oth | |
700 | 1 | |a Stroman, T. |4 oth | |
700 | 1 | |a Suzuki, S. |4 oth | |
700 | 1 | |a Takahashi, Y. |4 oth | |
700 | 1 | |a Takeda, M. |4 oth | |
700 | 1 | |a Taketa, A. |4 oth | |
700 | 1 | |a Takita, M. |4 oth | |
700 | 1 | |a Tameda, Y. |4 oth | |
700 | 1 | |a Tanaka, H. |4 oth | |
700 | 1 | |a Tanaka, K. |4 oth | |
700 | 1 | |a Tanaka, M. |4 oth | |
700 | 1 | |a Thomas, S.B. |4 oth | |
700 | 1 | |a Thomson, G.B. |4 oth | |
700 | 1 | |a Tinyakov, P. |4 oth | |
700 | 1 | |a Tkachev, I. |4 oth | |
700 | 1 | |a Tomida, T. |4 oth | |
700 | 1 | |a Troitsky, S. |4 oth | |
700 | 1 | |a Tsutsumi, K. |4 oth | |
700 | 1 | |a Tsuyuguchi, Y. |4 oth | |
700 | 1 | |a Uchihori, Y. |4 oth | |
700 | 1 | |a Udo, S. |4 oth | |
700 | 1 | |a Ukai, H. |4 oth | |
700 | 1 | |a Vasiloff, G. |4 oth | |
700 | 1 | |a Wada, Y. |4 oth | |
700 | 1 | |a Wong, T. |4 oth | |
700 | 1 | |a Wood, M. |4 oth | |
700 | 1 | |a Yamakawa, Y. |4 oth | |
700 | 1 | |a Yamane, R. |4 oth | |
700 | 1 | |a Yamaoka, H. |4 oth | |
700 | 1 | |a Yamazaki, K. |4 oth | |
700 | 1 | |a Yang, J. |4 oth | |
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700 | 1 | |a Zhou, X. |4 oth | |
700 | 1 | |a Zollinger, R. |4 oth | |
700 | 1 | |a Zundel, Z. |4 oth | |
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2014transfer abstract |
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44.90 |
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2014 |
allfields |
10.1016/j.nima.2014.09.059 doi GBVA2014006000003.pica (DE-627)ELV012130842 (ELSEVIER)S0168-9002(14)01090-0 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 44.90 bkl Shin, B.K. verfasserin aut Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation 2014transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. Ultra-high energy cosmic rays Elsevier Air fluorescence telescope Elsevier Calibration of photomultiplier Elsevier Tokuno, H. oth Tsunesada, Y. oth Abu-Zayyad, T. oth Aida, R. oth Allen, M. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, E.J. oth Cho, W.R. oth Fujii, H. oth Fujii, T. oth Fukuda, T. oth Fukushima, M. oth Hanlon, W. oth Hayashi, K. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Hiyama, K. oth Honda, K. oth Iguchi, T. oth Ikeda, D. oth Ikuta, K. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ivanov, D. oth Iwamoto, S. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kanbe, T. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kido, E. oth Kim, H.B. oth Kim, H.K. oth Kim, J.H. oth Kim, J.H. oth Kitamoto, K. oth Kitamura, S. oth Kitamura, Y. oth Kobayashi, K. oth Kobayashi, Y. oth Kondo, Y. oth Kuramoto, K. oth Kuzmin, V. oth Kwon, Y.J. oth Lim, S.I. oth Machida, S. oth Martens, K. oth Martineau, J. oth Matsuda, T. oth Matsuura, T. oth Matsuyama, T. oth Matthews, J.N. oth Myers, I. oth Minamino, M. oth Miyata, K. oth Murano, Y. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nam, S.W. oth Nonaka, T. oth Ogio, S. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Oku, D. oth Okuda, T. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Roh, S.Y. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, J.I. oth Shirahama, T. oth Smith, J.D. oth Sokolsky, P. oth Sonley, T.J. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T. oth Suzuki, S. oth Takahashi, Y. oth Takeda, M. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tomida, T. oth Troitsky, S. oth Tsutsumi, K. oth Tsuyuguchi, Y. oth Uchihori, Y. oth Udo, S. oth Ukai, H. oth Vasiloff, G. oth Wada, Y. oth Wong, T. oth Wood, M. oth Yamakawa, Y. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zhou, X. oth Zollinger, R. oth Zundel, Z. oth Enthalten in North-Holland Publ. Co Ide, C.V. ELSEVIER The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol 2017 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam (DE-627)ELV000874671 volume:768 year:2014 day:21 month:12 pages:96-103 extent:8 https://doi.org/10.1016/j.nima.2014.09.059 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.90 Neurologie VZ AR 768 2014 21 1221 96-103 8 045F 530 |
spelling |
10.1016/j.nima.2014.09.059 doi GBVA2014006000003.pica (DE-627)ELV012130842 (ELSEVIER)S0168-9002(14)01090-0 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 44.90 bkl Shin, B.K. verfasserin aut Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation 2014transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. Ultra-high energy cosmic rays Elsevier Air fluorescence telescope Elsevier Calibration of photomultiplier Elsevier Tokuno, H. oth Tsunesada, Y. oth Abu-Zayyad, T. oth Aida, R. oth Allen, M. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, E.J. oth Cho, W.R. oth Fujii, H. oth Fujii, T. oth Fukuda, T. oth Fukushima, M. oth Hanlon, W. oth Hayashi, K. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Hiyama, K. oth Honda, K. oth Iguchi, T. oth Ikeda, D. oth Ikuta, K. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ivanov, D. oth Iwamoto, S. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kanbe, T. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kido, E. oth Kim, H.B. oth Kim, H.K. oth Kim, J.H. oth Kim, J.H. oth Kitamoto, K. oth Kitamura, S. oth Kitamura, Y. oth Kobayashi, K. oth Kobayashi, Y. oth Kondo, Y. oth Kuramoto, K. oth Kuzmin, V. oth Kwon, Y.J. oth Lim, S.I. oth Machida, S. oth Martens, K. oth Martineau, J. oth Matsuda, T. oth Matsuura, T. oth Matsuyama, T. oth Matthews, J.N. oth Myers, I. oth Minamino, M. oth Miyata, K. oth Murano, Y. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nam, S.W. oth Nonaka, T. oth Ogio, S. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Oku, D. oth Okuda, T. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Roh, S.Y. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, J.I. oth Shirahama, T. oth Smith, J.D. oth Sokolsky, P. oth Sonley, T.J. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T. oth Suzuki, S. oth Takahashi, Y. oth Takeda, M. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tomida, T. oth Troitsky, S. oth Tsutsumi, K. oth Tsuyuguchi, Y. oth Uchihori, Y. oth Udo, S. oth Ukai, H. oth Vasiloff, G. oth Wada, Y. oth Wong, T. oth Wood, M. oth Yamakawa, Y. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zhou, X. oth Zollinger, R. oth Zundel, Z. oth Enthalten in North-Holland Publ. Co Ide, C.V. ELSEVIER The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol 2017 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam (DE-627)ELV000874671 volume:768 year:2014 day:21 month:12 pages:96-103 extent:8 https://doi.org/10.1016/j.nima.2014.09.059 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.90 Neurologie VZ AR 768 2014 21 1221 96-103 8 045F 530 |
allfields_unstemmed |
10.1016/j.nima.2014.09.059 doi GBVA2014006000003.pica (DE-627)ELV012130842 (ELSEVIER)S0168-9002(14)01090-0 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 44.90 bkl Shin, B.K. verfasserin aut Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation 2014transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. Ultra-high energy cosmic rays Elsevier Air fluorescence telescope Elsevier Calibration of photomultiplier Elsevier Tokuno, H. oth Tsunesada, Y. oth Abu-Zayyad, T. oth Aida, R. oth Allen, M. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, E.J. oth Cho, W.R. oth Fujii, H. oth Fujii, T. oth Fukuda, T. oth Fukushima, M. oth Hanlon, W. oth Hayashi, K. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Hiyama, K. oth Honda, K. oth Iguchi, T. oth Ikeda, D. oth Ikuta, K. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ivanov, D. oth Iwamoto, S. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kanbe, T. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kido, E. oth Kim, H.B. oth Kim, H.K. oth Kim, J.H. oth Kim, J.H. oth Kitamoto, K. oth Kitamura, S. oth Kitamura, Y. oth Kobayashi, K. oth Kobayashi, Y. oth Kondo, Y. oth Kuramoto, K. oth Kuzmin, V. oth Kwon, Y.J. oth Lim, S.I. oth Machida, S. oth Martens, K. oth Martineau, J. oth Matsuda, T. oth Matsuura, T. oth Matsuyama, T. oth Matthews, J.N. oth Myers, I. oth Minamino, M. oth Miyata, K. oth Murano, Y. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nam, S.W. oth Nonaka, T. oth Ogio, S. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Oku, D. oth Okuda, T. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Roh, S.Y. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, J.I. oth Shirahama, T. oth Smith, J.D. oth Sokolsky, P. oth Sonley, T.J. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T. oth Suzuki, S. oth Takahashi, Y. oth Takeda, M. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tomida, T. oth Troitsky, S. oth Tsutsumi, K. oth Tsuyuguchi, Y. oth Uchihori, Y. oth Udo, S. oth Ukai, H. oth Vasiloff, G. oth Wada, Y. oth Wong, T. oth Wood, M. oth Yamakawa, Y. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zhou, X. oth Zollinger, R. oth Zundel, Z. oth Enthalten in North-Holland Publ. Co Ide, C.V. ELSEVIER The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol 2017 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam (DE-627)ELV000874671 volume:768 year:2014 day:21 month:12 pages:96-103 extent:8 https://doi.org/10.1016/j.nima.2014.09.059 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.90 Neurologie VZ AR 768 2014 21 1221 96-103 8 045F 530 |
allfieldsGer |
10.1016/j.nima.2014.09.059 doi GBVA2014006000003.pica (DE-627)ELV012130842 (ELSEVIER)S0168-9002(14)01090-0 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 44.90 bkl Shin, B.K. verfasserin aut Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation 2014transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. Ultra-high energy cosmic rays Elsevier Air fluorescence telescope Elsevier Calibration of photomultiplier Elsevier Tokuno, H. oth Tsunesada, Y. oth Abu-Zayyad, T. oth Aida, R. oth Allen, M. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, E.J. oth Cho, W.R. oth Fujii, H. oth Fujii, T. oth Fukuda, T. oth Fukushima, M. oth Hanlon, W. oth Hayashi, K. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Hiyama, K. oth Honda, K. oth Iguchi, T. oth Ikeda, D. oth Ikuta, K. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ivanov, D. oth Iwamoto, S. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kanbe, T. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kido, E. oth Kim, H.B. oth Kim, H.K. oth Kim, J.H. oth Kim, J.H. oth Kitamoto, K. oth Kitamura, S. oth Kitamura, Y. oth Kobayashi, K. oth Kobayashi, Y. oth Kondo, Y. oth Kuramoto, K. oth Kuzmin, V. oth Kwon, Y.J. oth Lim, S.I. oth Machida, S. oth Martens, K. oth Martineau, J. oth Matsuda, T. oth Matsuura, T. oth Matsuyama, T. oth Matthews, J.N. oth Myers, I. oth Minamino, M. oth Miyata, K. oth Murano, Y. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nam, S.W. oth Nonaka, T. oth Ogio, S. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Oku, D. oth Okuda, T. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Roh, S.Y. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, J.I. oth Shirahama, T. oth Smith, J.D. oth Sokolsky, P. oth Sonley, T.J. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T. oth Suzuki, S. oth Takahashi, Y. oth Takeda, M. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tomida, T. oth Troitsky, S. oth Tsutsumi, K. oth Tsuyuguchi, Y. oth Uchihori, Y. oth Udo, S. oth Ukai, H. oth Vasiloff, G. oth Wada, Y. oth Wong, T. oth Wood, M. oth Yamakawa, Y. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zhou, X. oth Zollinger, R. oth Zundel, Z. oth Enthalten in North-Holland Publ. Co Ide, C.V. ELSEVIER The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol 2017 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam (DE-627)ELV000874671 volume:768 year:2014 day:21 month:12 pages:96-103 extent:8 https://doi.org/10.1016/j.nima.2014.09.059 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.90 Neurologie VZ AR 768 2014 21 1221 96-103 8 045F 530 |
allfieldsSound |
10.1016/j.nima.2014.09.059 doi GBVA2014006000003.pica (DE-627)ELV012130842 (ELSEVIER)S0168-9002(14)01090-0 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 44.90 bkl Shin, B.K. verfasserin aut Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation 2014transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. Ultra-high energy cosmic rays Elsevier Air fluorescence telescope Elsevier Calibration of photomultiplier Elsevier Tokuno, H. oth Tsunesada, Y. oth Abu-Zayyad, T. oth Aida, R. oth Allen, M. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, E.J. oth Cho, W.R. oth Fujii, H. oth Fujii, T. oth Fukuda, T. oth Fukushima, M. oth Hanlon, W. oth Hayashi, K. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Hiyama, K. oth Honda, K. oth Iguchi, T. oth Ikeda, D. oth Ikuta, K. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ivanov, D. oth Iwamoto, S. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kanbe, T. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kido, E. oth Kim, H.B. oth Kim, H.K. oth Kim, J.H. oth Kim, J.H. oth Kitamoto, K. oth Kitamura, S. oth Kitamura, Y. oth Kobayashi, K. oth Kobayashi, Y. oth Kondo, Y. oth Kuramoto, K. oth Kuzmin, V. oth Kwon, Y.J. oth Lim, S.I. oth Machida, S. oth Martens, K. oth Martineau, J. oth Matsuda, T. oth Matsuura, T. oth Matsuyama, T. oth Matthews, J.N. oth Myers, I. oth Minamino, M. oth Miyata, K. oth Murano, Y. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nam, S.W. oth Nonaka, T. oth Ogio, S. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Oku, D. oth Okuda, T. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Roh, S.Y. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, J.I. oth Shirahama, T. oth Smith, J.D. oth Sokolsky, P. oth Sonley, T.J. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T. oth Suzuki, S. oth Takahashi, Y. oth Takeda, M. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tomida, T. oth Troitsky, S. oth Tsutsumi, K. oth Tsuyuguchi, Y. oth Uchihori, Y. oth Udo, S. oth Ukai, H. oth Vasiloff, G. oth Wada, Y. oth Wong, T. oth Wood, M. oth Yamakawa, Y. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zhou, X. oth Zollinger, R. oth Zundel, Z. oth Enthalten in North-Holland Publ. Co Ide, C.V. ELSEVIER The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol 2017 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam (DE-627)ELV000874671 volume:768 year:2014 day:21 month:12 pages:96-103 extent:8 https://doi.org/10.1016/j.nima.2014.09.059 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.90 Neurologie VZ AR 768 2014 21 1221 96-103 8 045F 530 |
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The efficacy of EEG-biofeedback for acute pain management, a randomized sham-controlled study of a tailored protocol |
authorswithroles_txt_mv |
Shin, B.K. @@aut@@ Tokuno, H. @@oth@@ Tsunesada, Y. @@oth@@ Abu-Zayyad, T. @@oth@@ Aida, R. @@oth@@ Allen, M. @@oth@@ Anderson, R. @@oth@@ Azuma, R. @@oth@@ Barcikowski, E. @@oth@@ Belz, J.W. @@oth@@ Bergman, D.R. @@oth@@ Blake, S.A. @@oth@@ Cady, R. @@oth@@ Cheon, B.G. @@oth@@ Chiba, J. @@oth@@ Chikawa, M. @@oth@@ Cho, E.J. @@oth@@ Cho, W.R. @@oth@@ Fujii, H. @@oth@@ Fujii, T. @@oth@@ Fukuda, T. @@oth@@ Fukushima, M. @@oth@@ Hanlon, W. @@oth@@ Hayashi, K. @@oth@@ Hayashi, Y. @@oth@@ Hayashida, N. @@oth@@ Hibino, K. @@oth@@ Hiyama, K. @@oth@@ Honda, K. @@oth@@ Iguchi, T. @@oth@@ Ikeda, D. @@oth@@ Ikuta, K. @@oth@@ Inoue, N. @@oth@@ Ishii, T. @@oth@@ Ishimori, R. @@oth@@ Ivanov, D. @@oth@@ Iwamoto, S. @@oth@@ Jui, C.C.H. @@oth@@ Kadota, K. @@oth@@ Kakimoto, F. @@oth@@ Kalashev, O. @@oth@@ Kanbe, T. @@oth@@ Kasahara, K. @@oth@@ Kawai, H. @@oth@@ Kawakami, S. @@oth@@ Kawana, S. @@oth@@ Kido, E. @@oth@@ Kim, H.B. @@oth@@ Kim, H.K. @@oth@@ Kim, J.H. @@oth@@ Kitamoto, K. @@oth@@ Kitamura, S. @@oth@@ Kitamura, Y. @@oth@@ Kobayashi, K. @@oth@@ Kobayashi, Y. @@oth@@ Kondo, Y. @@oth@@ Kuramoto, K. @@oth@@ Kuzmin, V. @@oth@@ Kwon, Y.J. @@oth@@ Lim, S.I. @@oth@@ Machida, S. @@oth@@ Martens, K. @@oth@@ Martineau, J. @@oth@@ Matsuda, T. @@oth@@ Matsuura, T. @@oth@@ Matsuyama, T. @@oth@@ Matthews, J.N. @@oth@@ Myers, I. @@oth@@ Minamino, M. @@oth@@ Miyata, K. @@oth@@ Murano, Y. @@oth@@ Nagasawa, K. @@oth@@ Nagataki, S. @@oth@@ Nakamura, T. @@oth@@ Nam, S.W. @@oth@@ Nonaka, T. @@oth@@ Ogio, S. @@oth@@ Ohnishi, M. @@oth@@ Ohoka, H. @@oth@@ Oki, K. @@oth@@ Oku, D. @@oth@@ Okuda, T. @@oth@@ Oshima, A. @@oth@@ Ozawa, S. @@oth@@ Park, I.H. @@oth@@ Pshirkov, M.S. @@oth@@ Rodriguez, D.C. @@oth@@ Roh, S.Y. @@oth@@ Rubtsov, G. @@oth@@ Ryu, D. @@oth@@ Sagawa, H. @@oth@@ Sakurai, N. @@oth@@ Sampson, A.L. @@oth@@ Scott, L.M. @@oth@@ Shah, P.D. @@oth@@ Shibata, F. @@oth@@ Shibata, T. @@oth@@ Shimodaira, H. @@oth@@ Shin, J.I. @@oth@@ Shirahama, T. @@oth@@ Smith, J.D. @@oth@@ Sokolsky, P. @@oth@@ Sonley, T.J. @@oth@@ Springer, R.W. @@oth@@ Stokes, B.T. @@oth@@ Stratton, S.R. @@oth@@ Stroman, T. @@oth@@ Suzuki, S. @@oth@@ Takahashi, Y. @@oth@@ Takeda, M. @@oth@@ Taketa, A. @@oth@@ Takita, M. @@oth@@ Tameda, Y. @@oth@@ Tanaka, H. @@oth@@ Tanaka, K. @@oth@@ Tanaka, M. @@oth@@ Thomas, S.B. @@oth@@ Thomson, G.B. @@oth@@ Tinyakov, P. @@oth@@ Tkachev, I. @@oth@@ Tomida, T. @@oth@@ Troitsky, S. @@oth@@ Tsutsumi, K. @@oth@@ Tsuyuguchi, Y. @@oth@@ Uchihori, Y. @@oth@@ Udo, S. @@oth@@ Ukai, H. @@oth@@ Vasiloff, G. @@oth@@ Wada, Y. @@oth@@ Wong, T. @@oth@@ Wood, M. @@oth@@ Yamakawa, Y. @@oth@@ Yamane, R. @@oth@@ Yamaoka, H. @@oth@@ Yamazaki, K. @@oth@@ Yang, J. @@oth@@ Yoneda, Y. @@oth@@ Yoshida, S. @@oth@@ Yoshii, H. @@oth@@ Zhou, X. @@oth@@ Zollinger, R. @@oth@@ Zundel, Z. @@oth@@ |
publishDateDaySort_date |
2014-01-21T00:00:00Z |
hierarchy_top_id |
ELV000874671 |
dewey-sort |
3530 |
id |
ELV012130842 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV012130842</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230625110415.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">180602s2014 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.nima.2014.09.059</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">GBVA2014006000003.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV012130842</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0168-9002(14)01090-0</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">530</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">610</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">44.90</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Shin, B.K.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">8</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Ultra-high energy cosmic rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Air fluorescence telescope</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Calibration of photomultiplier</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tokuno, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsunesada, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abu-Zayyad, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aida, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Allen, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anderson, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Azuma, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barcikowski, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belz, J.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bergman, D.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blake, S.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cady, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cheon, B.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chiba, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chikawa, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cho, E.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cho, W.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fujii, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fujii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fukuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fukushima, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hanlon, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashi, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashi, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashida, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hibino, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hiyama, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Honda, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Iguchi, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ikeda, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ikuta, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Inoue, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishimori, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ivanov, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Iwamoto, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jui, C.C.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kadota, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kakimoto, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kalashev, O.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kanbe, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kasahara, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawai, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawakami, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawana, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kido, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, H.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, H.K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamoto, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kobayashi, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kobayashi, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kondo, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuramoto, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuzmin, V.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kwon, Y.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lim, 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code="a">Nonaka, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ogio, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohnishi, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohoka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oki, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oku, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Okuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oshima, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ozawa, 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N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sampson, A.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Scott, L.M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shah, P.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shimodaira, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shin, J.I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield 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gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation |
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Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation |
abstract |
The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. |
abstractGer |
The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. |
abstract_unstemmed |
The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year. |
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Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation |
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https://doi.org/10.1016/j.nima.2014.09.059 |
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Tokuno, H. Tsunesada, Y. Abu-Zayyad, T. Aida, R. Allen, M. Anderson, R. Azuma, R. Barcikowski, E. Belz, J.W. Bergman, D.R. Blake, S.A. Cady, R. Cheon, B.G. Chiba, J. Chikawa, M. Cho, E.J. Cho, W.R. Fujii, H. Fujii, T. Fukuda, T. Fukushima, M. Hanlon, W. Hayashi, K. Hayashi, Y. Hayashida, N. Hibino, K. Hiyama, K. Honda, K. Iguchi, T. Ikeda, D. Ikuta, K. Inoue, N. Ishii, T. Ishimori, R. Ivanov, D. Iwamoto, S. Jui, C.C.H. Kadota, K. Kakimoto, F. Kalashev, O. Kanbe, T. Kasahara, K. Kawai, H. Kawakami, S. Kawana, S. Kido, E. Kim, H.B. Kim, H.K. Kim, J.H. Kitamoto, K. Kitamura, S. Kitamura, Y. Kobayashi, K. Kobayashi, Y. Kondo, Y. Kuramoto, K. Kuzmin, V. Kwon, Y.J. Lim, S.I. Machida, S. Martens, K. Martineau, J. Matsuda, T. Matsuura, T. Matsuyama, T. Matthews, J.N. Myers, I. Minamino, M. Miyata, K. Murano, Y. Nagasawa, K. Nagataki, S. Nakamura, T. Nam, S.W. Nonaka, T. Ogio, S. Ohnishi, M. Ohoka, H. Oki, K. Oku, D. Okuda, T. Oshima, A. Ozawa, S. Park, I.H. Pshirkov, M.S. Rodriguez, D.C. Roh, S.Y. Rubtsov, G. Ryu, D. Sagawa, H. Sakurai, N. Sampson, A.L. Scott, L.M. Shah, P.D. Shibata, F. Shibata, T. Shimodaira, H. Shin, J.I. Shirahama, T. Smith, J.D. Sokolsky, P. Sonley, T.J. Springer, R.W. Stokes, B.T. Stratton, S.R. Stroman, T. Suzuki, S. Takahashi, Y. Takeda, M. Taketa, A. Takita, M. Tameda, Y. Tanaka, H. Tanaka, K. Tanaka, M. Thomas, S.B. Thomson, G.B. Tinyakov, P. Tkachev, I. Tomida, T. Troitsky, S. Tsutsumi, K. Tsuyuguchi, Y. Uchihori, Y. Udo, S. Ukai, H. Vasiloff, G. Wada, Y. Wong, T. Wood, M. Yamakawa, Y. Yamane, R. Yamaoka, H. Yamazaki, K. Yang, J. Yoneda, Y. Yoshida, S. Yoshii, H. Zhou, X. Zollinger, R. Zundel, Z. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV012130842</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230625110415.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">180602s2014 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.nima.2014.09.059</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">GBVA2014006000003.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV012130842</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0168-9002(14)01090-0</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">530</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">610</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">44.90</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Shin, B.K.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">8</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Ultra-high energy cosmic rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Air fluorescence telescope</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Calibration of photomultiplier</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tokuno, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsunesada, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abu-Zayyad, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aida, 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