Position reconstruction in LUX
| Publication Date: |
2018-02-02
|
|---|---|
| Publisher: |
Institute of Physics Publishing (IOP)
|
| Electronic ISSN: |
1748-0221
|
| Topics: |
Physics
|
| Published by: |
| _version_ | 1836398772436860928 |
|---|---|
| autor | D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang |
| beschreibung | The ( x, y ) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented. The algorithm is based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data. The light response functions make use of a two dimensional functional form to account for the photons reflected on the inner walls of the detector. To increase the resolution for small pulses, a photon counting technique was employed to describe the response of the PMTs. The reconstruction was assessed with calibration data including 83m Kr (releasing a total energy of 41.5 keV) and 3 H (β − with Q = 18.6 keV) decays, and a deuterium-deuterium (D-D) neutron beam (2.45 MeV) . Within the detector's fiducial volume, the reconstruction has achieved an ( x, y ) position uncertainty of σ = 0.82 cm and ... |
| citation_standardnr | 6152168 |
| datenlieferant | ipn_articles |
| feed_id | 66992 |
| feed_publisher | Institute of Physics Publishing (IOP) |
| feed_publisher_url | http://www.iop.org/ |
| insertion_date | 2018-02-02 |
| journaleissn | 1748-0221 |
| publikationsjahr_anzeige | 2018 |
| publikationsjahr_facette | 2018 |
| publikationsjahr_intervall | 7984:2015-2019 |
| publikationsjahr_sort | 2018 |
| publisher | Institute of Physics Publishing (IOP) |
| quelle | Journal of Instrumentation |
| relation | http://iopscience.iop.org/1748-0221/13/02/P02001 |
| search_space | articles |
| shingle_author_1 | D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang |
| shingle_author_2 | D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang |
| shingle_author_3 | D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang |
| shingle_author_4 | D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang |
| shingle_catch_all_1 | Position reconstruction in LUX The ( x, y ) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented. The algorithm is based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data. The light response functions make use of a two dimensional functional form to account for the photons reflected on the inner walls of the detector. To increase the resolution for small pulses, a photon counting technique was employed to describe the response of the PMTs. The reconstruction was assessed with calibration data including 83m Kr (releasing a total energy of 41.5 keV) and 3 H (β − with Q = 18.6 keV) decays, and a deuterium-deuterium (D-D) neutron beam (2.45 MeV) . Within the detector's fiducial volume, the reconstruction has achieved an ( x, y ) position uncertainty of σ = 0.82 cm and ... D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang Institute of Physics Publishing (IOP) 1748-0221 17480221 |
| shingle_catch_all_2 | Position reconstruction in LUX The ( x, y ) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented. The algorithm is based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data. The light response functions make use of a two dimensional functional form to account for the photons reflected on the inner walls of the detector. To increase the resolution for small pulses, a photon counting technique was employed to describe the response of the PMTs. The reconstruction was assessed with calibration data including 83m Kr (releasing a total energy of 41.5 keV) and 3 H (β − with Q = 18.6 keV) decays, and a deuterium-deuterium (D-D) neutron beam (2.45 MeV) . Within the detector's fiducial volume, the reconstruction has achieved an ( x, y ) position uncertainty of σ = 0.82 cm and ... D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang Institute of Physics Publishing (IOP) 1748-0221 17480221 |
| shingle_catch_all_3 | Position reconstruction in LUX The ( x, y ) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented. The algorithm is based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data. The light response functions make use of a two dimensional functional form to account for the photons reflected on the inner walls of the detector. To increase the resolution for small pulses, a photon counting technique was employed to describe the response of the PMTs. The reconstruction was assessed with calibration data including 83m Kr (releasing a total energy of 41.5 keV) and 3 H (β − with Q = 18.6 keV) decays, and a deuterium-deuterium (D-D) neutron beam (2.45 MeV) . Within the detector's fiducial volume, the reconstruction has achieved an ( x, y ) position uncertainty of σ = 0.82 cm and ... D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang Institute of Physics Publishing (IOP) 1748-0221 17480221 |
| shingle_catch_all_4 | Position reconstruction in LUX The ( x, y ) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented. The algorithm is based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data. The light response functions make use of a two dimensional functional form to account for the photons reflected on the inner walls of the detector. To increase the resolution for small pulses, a photon counting technique was employed to describe the response of the PMTs. The reconstruction was assessed with calibration data including 83m Kr (releasing a total energy of 41.5 keV) and 3 H (β − with Q = 18.6 keV) decays, and a deuterium-deuterium (D-D) neutron beam (2.45 MeV) . Within the detector's fiducial volume, the reconstruction has achieved an ( x, y ) position uncertainty of σ = 0.82 cm and ... D.S. Akerib, S. Alsum, H.M. Araújo, X. Bai, A.J. Bailey, J. Balajthy, P. Beltrame, E.P. Bernard, A. Bernstein, T.P. Biesiadzinski, E.M. Boulton, P. Brás, D. Byram, S.B. Cahn, M.C. Carmona-Benitez, C. Chan, A. Currie, J.E. Cutter, T.J.R. Davison, A. Dobi, E. Druszkiewicz, B.N. Edwards, S.R. Fallon, A. Fan, S. Fiorucci, R.J. Gaitskell, J. Genovesi, C. Ghag, M.G.D. Gilchriese, C.R. Hall, M. Hanhardt, S.J. Haselschwardt, S.A. Hertel, D.P. Hogan, M. Horn, D.Q. Huang, C.M. Ignarra, R.G. Jacobsen, W. Ji, K. Kamdin, K. Kazkaz, D. Khaitan, R. Knoche, N.A. Larsen, B.G. Lenardo, K.T. Lesko, A. Lindote, M.I. Lopes, A. Manalaysay, R.L. Mannino, M.F. Marzioni, D.N. McKinsey, D.-M. Mei, J. Mock, M. Moongweluwan, J.A. Morad, A.St.J. Murphy, C. Nehrkorn, H.N. Nelson, F. Neves, K. O'Sullivan, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, C. Rhyne, S. Shaw, T.A. Shutt, C. Silva, M. Solmaz, V.N. Solovov, P. Sorensen, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, B.P. Tennyson, P.A. Terman, D.R. Tiedt, W.H. To, M. Tripathi, L. Tvrznikova, S. Uvarov, V. Velan, J.R. Verbus, R.C. Webb, J.T. White, T.J. Whitis, M.S. Witherell, F.L.H. Wolfs, J. Xu, K. Yazdani, S.K. Young and C. Zhang Institute of Physics Publishing (IOP) 1748-0221 17480221 |
| shingle_title_1 | Position reconstruction in LUX |
| shingle_title_2 | Position reconstruction in LUX |
| shingle_title_3 | Position reconstruction in LUX |
| shingle_title_4 | Position reconstruction in LUX |
| timestamp | 2025-06-30T23:32:23.779Z |
| titel | Position reconstruction in LUX |
| titel_suche | Position reconstruction in LUX |
| topic | U |
| uid | ipn_articles_6152168 |