The data acquisition system of the LZ dark matter detector: FADR
The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MHz 32-channel digitizers (DDC-32s). A basic waveform analysis is carried out on the on-board Field Programmable Gate Arra...
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Veröffentlicht in: | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Accelerators, spectrometers, detectors and associated equipment, 2024-11, Vol.1068, p.169712, Article 169712 |
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creator | Aalbers, J. Al Musalhi, A.K. Amarasinghe, C.S. Araújo, H.M. Armstrong, J.E. Baker, A. Balashov, S. Bang, J. Beattie, K. Boxer, B. Brew, C.A.J. Brás, P. Buckley, J.H. Burdin, S. Carmona-Benitez, M.C. Chin, Y.T. Cottle, A. Cox, G. Curran, D. Dahl, C.E. David, A. de Viveiros, L. Dimino, T. Dobson, J.E.Y. Fiorucci, S. Fraser, E.D. Fruth, T.M.A. Geffre, A. Gelfand, R. Ghag, C. Gokhale, S. van der Grinten, M.G.D. Haiston, J.J. Hall, C.R. Han, S. James, R.S. Kamaha, A.C. Khaitan, D. Khazov, A. Khurana, I. Kim, J. Kingston, J. Kodroff, D. Korley, L. Leonard, D.S. Lesko, K.T. Levy, C. Lorenzon, W. Majewski, P.A. Manalaysay, A. Mannino, R.L. McDowell, G. McLaughlin, J. McMonigle, R. Mizrachi, E. Monzani, M.E. Moongweluwan, M. Morrison, E. Mount, B.J. Murdy, M. Neves, F. Nikoleyczik, J.A. Olevitch, M.A. Oliver-Mallory, K.C. Orpwood, J. Palmer, J. Pannifer, N.J. Pereira, G. Pershing, T. Piepke, A. Reichenbacher, J. Rhyne, C.A. Riyat, H.S. Rushton, T. Schnee, R.W. Shaw, S. Silva, C. Siniscalco, J. Skulski, W. Smith, R. Solovov, V.N. Sorensen, P. Soria, J. Stancu, I. Sumner, T.J. Szydagis, M. Timalsina, M. Tovey, D.R. Tranter, J. Tripathi, M. Vacheret, A. Vaitkus, A.C. Valentino, O. Watson, J.R. Williams, M. Wolfs, J.D. Wright, C.J. Xia, Q. Xiang, X. Yin, J. |
description | The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MHz 32-channel digitizers (DDC-32s). A basic waveform analysis is carried out on the on-board Field Programmable Gate Arrays (FPGAs) to extract information about the observed scintillation and electroluminescence signals. This information is used to determine if the digitized waveforms should be preserved for offline analysis.
The system is designed around the Kintex-7 FPGA. In addition to digitizing the PMT signals and providing basic event selection in real time, the flexibility provided by the use of FPGAs allows us to monitor the performance of the detector and the DAQ in parallel to normal data acquisition.
The hardware and software/firmware of this FPGA-based Architecture for Data acquisition and Realtime monitoring (FADR) are discussed and performance measurements are described. |
doi_str_mv | 10.1016/j.nima.2024.169712 |
format | Article |
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The system is designed around the Kintex-7 FPGA. In addition to digitizing the PMT signals and providing basic event selection in real time, the flexibility provided by the use of FPGAs allows us to monitor the performance of the detector and the DAQ in parallel to normal data acquisition.
The hardware and software/firmware of this FPGA-based Architecture for Data acquisition and Realtime monitoring (FADR) are discussed and performance measurements are described.</description><identifier>ISSN: 0168-9002</identifier><identifier>DOI: 10.1016/j.nima.2024.169712</identifier><language>eng</language><publisher>United States: Elsevier B.V</publisher><subject>Dark matter ; Data acquisition ; Firmware ; FPGA</subject><ispartof>Nuclear instruments & methods in physics research. 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J.</creatorcontrib><creatorcontrib>Tripathi, M.</creatorcontrib><creatorcontrib>Vacheret, A.</creatorcontrib><creatorcontrib>Vaitkus, A.C.</creatorcontrib><creatorcontrib>Valentino, O.</creatorcontrib><creatorcontrib>Watson, J.R.</creatorcontrib><creatorcontrib>Williams, M.</creatorcontrib><creatorcontrib>Wolfs, J.D.</creatorcontrib><creatorcontrib>Wright, C.J.</creatorcontrib><creatorcontrib>Xia, Q.</creatorcontrib><creatorcontrib>Xiang, X.</creatorcontrib><creatorcontrib>Yin, J.</creatorcontrib><creatorcontrib>Univ. of Rochester, NY (United States)</creatorcontrib><title>The data acquisition system of the LZ dark matter detector: FADR</title><title>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</title><description>The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MHz 32-channel digitizers (DDC-32s). A basic waveform analysis is carried out on the on-board Field Programmable Gate Arrays (FPGAs) to extract information about the observed scintillation and electroluminescence signals. This information is used to determine if the digitized waveforms should be preserved for offline analysis.
The system is designed around the Kintex-7 FPGA. In addition to digitizing the PMT signals and providing basic event selection in real time, the flexibility provided by the use of FPGAs allows us to monitor the performance of the detector and the DAQ in parallel to normal data acquisition.
The hardware and software/firmware of this FPGA-based Architecture for Data acquisition and Realtime monitoring (FADR) are discussed and performance measurements are described.</description><subject>Dark matter</subject><subject>Data acquisition</subject><subject>Firmware</subject><subject>FPGA</subject><issn>0168-9002</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNp9kE9LxDAQxXNQcF39Ap6C99ZJ2qapeHBZXRUKgqwXLyGbP2xWt9EkCvvtTaln5zIM897j8UPogkBJgLCrXTm4vSwp0LokrGsJPUKz_OBFB0BP0GmMO8jTtXyGbtdbg7VMEkv19e2iS84POB5iMnvsLU753b9lRXjHe5mSCVibZFTy4RqvFncvZ-jYyo9ozv_2HL2u7tfLx6J_fnhaLvpC0YamgvPGso2mrGG8krQjRiudT95AZRVsgLPWtrq2Ha-7mjIARqHmlVLaAGx0NUeXU66PyYmoXC6xVX4YchdB65bThmQRnUQq-BiDseIzZBbhIAiIEY7YiRGOGOGICU423Uwmk-v_OBPGdDMoo10Yw7V3_9l_AXgubVU</recordid><startdate>20241101</startdate><enddate>20241101</enddate><creator>Aalbers, J.</creator><creator>Al Musalhi, A.K.</creator><creator>Amarasinghe, 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J.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-8693-1196</orcidid><orcidid>https://orcid.org/0000000186931196</orcidid></search><sort><creationdate>20241101</creationdate><title>The data acquisition system of the LZ dark matter detector: FADR</title><author>Aalbers, J. ; Al Musalhi, A.K. ; Amarasinghe, C.S. ; Araújo, H.M. ; Armstrong, J.E. ; Baker, A. ; Balashov, S. ; Bang, J. ; Beattie, K. ; Boxer, B. ; Brew, C.A.J. ; Brás, P. ; Buckley, J.H. ; Burdin, S. ; Carmona-Benitez, M.C. ; Chin, Y.T. ; Cottle, A. ; Cox, G. ; Curran, D. ; Dahl, C.E. ; David, A. ; de Viveiros, L. ; Dimino, T. ; Dobson, J.E.Y. ; Fiorucci, S. ; Fraser, E.D. ; Fruth, T.M.A. ; Geffre, A. ; Gelfand, R. ; Ghag, C. ; Gokhale, S. ; van der Grinten, M.G.D. ; Haiston, J.J. ; Hall, C.R. ; Han, S. ; James, R.S. ; Kamaha, A.C. ; Khaitan, D. ; Khazov, A. ; Khurana, I. ; Kim, J. ; Kingston, J. ; Kodroff, D. ; Korley, L. ; Leonard, D.S. ; Lesko, K.T. ; Levy, C. ; Lorenzon, W. ; Majewski, P.A. ; Manalaysay, A. ; Mannino, R.L. ; McDowell, G. ; McLaughlin, J. ; McMonigle, R. ; Mizrachi, E. ; Monzani, M.E. ; Moongweluwan, M. ; Morrison, E. ; Mount, B.J. ; Murdy, M. ; Neves, F. ; Nikoleyczik, J.A. ; Olevitch, M.A. ; Oliver-Mallory, K.C. ; Orpwood, J. ; Palmer, J. ; Pannifer, N.J. ; Pereira, G. ; Pershing, T. ; Piepke, A. ; Reichenbacher, J. ; Rhyne, C.A. ; Riyat, H.S. ; Rushton, T. ; Schnee, R.W. ; Shaw, S. ; Silva, C. ; Siniscalco, J. ; Skulski, W. ; Smith, R. ; Solovov, V.N. ; Sorensen, P. ; Soria, J. ; Stancu, I. ; Sumner, T.J. ; Szydagis, M. ; Timalsina, M. ; Tovey, D.R. ; Tranter, J. ; Tripathi, M. ; Vacheret, A. ; Vaitkus, A.C. ; Valentino, O. ; Watson, J.R. ; Williams, M. ; Wolfs, J.D. ; Wright, C.J. ; Xia, Q. ; Xiang, X. ; Yin, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c252t-885f6bd265683a291edcdd268503fc0b0867f7d4f984942600620483ccde00bd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Dark matter</topic><topic>Data acquisition</topic><topic>Firmware</topic><topic>FPGA</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Aalbers, J.</creatorcontrib><creatorcontrib>Al Musalhi, A.K.</creatorcontrib><creatorcontrib>Amarasinghe, C.S.</creatorcontrib><creatorcontrib>Araújo, H.M.</creatorcontrib><creatorcontrib>Armstrong, J.E.</creatorcontrib><creatorcontrib>Baker, A.</creatorcontrib><creatorcontrib>Balashov, S.</creatorcontrib><creatorcontrib>Bang, J.</creatorcontrib><creatorcontrib>Beattie, K.</creatorcontrib><creatorcontrib>Boxer, B.</creatorcontrib><creatorcontrib>Brew, C.A.J.</creatorcontrib><creatorcontrib>Brás, P.</creatorcontrib><creatorcontrib>Buckley, J.H.</creatorcontrib><creatorcontrib>Burdin, S.</creatorcontrib><creatorcontrib>Carmona-Benitez, M.C.</creatorcontrib><creatorcontrib>Chin, Y.T.</creatorcontrib><creatorcontrib>Cottle, A.</creatorcontrib><creatorcontrib>Cox, G.</creatorcontrib><creatorcontrib>Curran, D.</creatorcontrib><creatorcontrib>Dahl, C.E.</creatorcontrib><creatorcontrib>David, A.</creatorcontrib><creatorcontrib>de Viveiros, L.</creatorcontrib><creatorcontrib>Dimino, T.</creatorcontrib><creatorcontrib>Dobson, J.E.Y.</creatorcontrib><creatorcontrib>Fiorucci, S.</creatorcontrib><creatorcontrib>Fraser, E.D.</creatorcontrib><creatorcontrib>Fruth, T.M.A.</creatorcontrib><creatorcontrib>Geffre, A.</creatorcontrib><creatorcontrib>Gelfand, R.</creatorcontrib><creatorcontrib>Ghag, C.</creatorcontrib><creatorcontrib>Gokhale, S.</creatorcontrib><creatorcontrib>van der Grinten, M.G.D.</creatorcontrib><creatorcontrib>Haiston, J.J.</creatorcontrib><creatorcontrib>Hall, C.R.</creatorcontrib><creatorcontrib>Han, S.</creatorcontrib><creatorcontrib>James, R.S.</creatorcontrib><creatorcontrib>Kamaha, A.C.</creatorcontrib><creatorcontrib>Khaitan, D.</creatorcontrib><creatorcontrib>Khazov, A.</creatorcontrib><creatorcontrib>Khurana, I.</creatorcontrib><creatorcontrib>Kim, J.</creatorcontrib><creatorcontrib>Kingston, J.</creatorcontrib><creatorcontrib>Kodroff, D.</creatorcontrib><creatorcontrib>Korley, L.</creatorcontrib><creatorcontrib>Leonard, D.S.</creatorcontrib><creatorcontrib>Lesko, K.T.</creatorcontrib><creatorcontrib>Levy, C.</creatorcontrib><creatorcontrib>Lorenzon, W.</creatorcontrib><creatorcontrib>Majewski, P.A.</creatorcontrib><creatorcontrib>Manalaysay, A.</creatorcontrib><creatorcontrib>Mannino, R.L.</creatorcontrib><creatorcontrib>McDowell, G.</creatorcontrib><creatorcontrib>McLaughlin, J.</creatorcontrib><creatorcontrib>McMonigle, R.</creatorcontrib><creatorcontrib>Mizrachi, E.</creatorcontrib><creatorcontrib>Monzani, M.E.</creatorcontrib><creatorcontrib>Moongweluwan, M.</creatorcontrib><creatorcontrib>Morrison, E.</creatorcontrib><creatorcontrib>Mount, B.J.</creatorcontrib><creatorcontrib>Murdy, M.</creatorcontrib><creatorcontrib>Neves, F.</creatorcontrib><creatorcontrib>Nikoleyczik, J.A.</creatorcontrib><creatorcontrib>Olevitch, M.A.</creatorcontrib><creatorcontrib>Oliver-Mallory, K.C.</creatorcontrib><creatorcontrib>Orpwood, J.</creatorcontrib><creatorcontrib>Palmer, J.</creatorcontrib><creatorcontrib>Pannifer, N.J.</creatorcontrib><creatorcontrib>Pereira, G.</creatorcontrib><creatorcontrib>Pershing, T.</creatorcontrib><creatorcontrib>Piepke, A.</creatorcontrib><creatorcontrib>Reichenbacher, J.</creatorcontrib><creatorcontrib>Rhyne, C.A.</creatorcontrib><creatorcontrib>Riyat, H.S.</creatorcontrib><creatorcontrib>Rushton, T.</creatorcontrib><creatorcontrib>Schnee, R.W.</creatorcontrib><creatorcontrib>Shaw, S.</creatorcontrib><creatorcontrib>Silva, C.</creatorcontrib><creatorcontrib>Siniscalco, J.</creatorcontrib><creatorcontrib>Skulski, W.</creatorcontrib><creatorcontrib>Smith, R.</creatorcontrib><creatorcontrib>Solovov, V.N.</creatorcontrib><creatorcontrib>Sorensen, P.</creatorcontrib><creatorcontrib>Soria, J.</creatorcontrib><creatorcontrib>Stancu, I.</creatorcontrib><creatorcontrib>Sumner, T.J.</creatorcontrib><creatorcontrib>Szydagis, M.</creatorcontrib><creatorcontrib>Timalsina, M.</creatorcontrib><creatorcontrib>Tovey, D.R.</creatorcontrib><creatorcontrib>Tranter, J.</creatorcontrib><creatorcontrib>Tripathi, M.</creatorcontrib><creatorcontrib>Vacheret, A.</creatorcontrib><creatorcontrib>Vaitkus, A.C.</creatorcontrib><creatorcontrib>Valentino, O.</creatorcontrib><creatorcontrib>Watson, J.R.</creatorcontrib><creatorcontrib>Williams, M.</creatorcontrib><creatorcontrib>Wolfs, J.D.</creatorcontrib><creatorcontrib>Wright, C.J.</creatorcontrib><creatorcontrib>Xia, Q.</creatorcontrib><creatorcontrib>Xiang, X.</creatorcontrib><creatorcontrib>Yin, J.</creatorcontrib><creatorcontrib>Univ. of Rochester, NY (United States)</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aalbers, J.</au><au>Al Musalhi, A.K.</au><au>Amarasinghe, C.S.</au><au>Araújo, H.M.</au><au>Armstrong, J.E.</au><au>Baker, A.</au><au>Balashov, S.</au><au>Bang, J.</au><au>Beattie, K.</au><au>Boxer, B.</au><au>Brew, C.A.J.</au><au>Brás, P.</au><au>Buckley, J.H.</au><au>Burdin, S.</au><au>Carmona-Benitez, M.C.</au><au>Chin, Y.T.</au><au>Cottle, A.</au><au>Cox, G.</au><au>Curran, D.</au><au>Dahl, C.E.</au><au>David, A.</au><au>de Viveiros, L.</au><au>Dimino, T.</au><au>Dobson, J.E.Y.</au><au>Fiorucci, S.</au><au>Fraser, E.D.</au><au>Fruth, T.M.A.</au><au>Geffre, A.</au><au>Gelfand, R.</au><au>Ghag, C.</au><au>Gokhale, S.</au><au>van der Grinten, M.G.D.</au><au>Haiston, J.J.</au><au>Hall, C.R.</au><au>Han, S.</au><au>James, R.S.</au><au>Kamaha, A.C.</au><au>Khaitan, D.</au><au>Khazov, A.</au><au>Khurana, I.</au><au>Kim, J.</au><au>Kingston, J.</au><au>Kodroff, D.</au><au>Korley, L.</au><au>Leonard, D.S.</au><au>Lesko, K.T.</au><au>Levy, C.</au><au>Lorenzon, W.</au><au>Majewski, P.A.</au><au>Manalaysay, A.</au><au>Mannino, R.L.</au><au>McDowell, G.</au><au>McLaughlin, J.</au><au>McMonigle, R.</au><au>Mizrachi, E.</au><au>Monzani, M.E.</au><au>Moongweluwan, M.</au><au>Morrison, E.</au><au>Mount, B.J.</au><au>Murdy, M.</au><au>Neves, F.</au><au>Nikoleyczik, J.A.</au><au>Olevitch, M.A.</au><au>Oliver-Mallory, K.C.</au><au>Orpwood, J.</au><au>Palmer, J.</au><au>Pannifer, N.J.</au><au>Pereira, G.</au><au>Pershing, T.</au><au>Piepke, A.</au><au>Reichenbacher, J.</au><au>Rhyne, C.A.</au><au>Riyat, H.S.</au><au>Rushton, T.</au><au>Schnee, R.W.</au><au>Shaw, S.</au><au>Silva, C.</au><au>Siniscalco, J.</au><au>Skulski, W.</au><au>Smith, R.</au><au>Solovov, V.N.</au><au>Sorensen, P.</au><au>Soria, J.</au><au>Stancu, I.</au><au>Sumner, T.J.</au><au>Szydagis, M.</au><au>Timalsina, M.</au><au>Tovey, D.R.</au><au>Tranter, J.</au><au>Tripathi, M.</au><au>Vacheret, A.</au><au>Vaitkus, A.C.</au><au>Valentino, O.</au><au>Watson, J.R.</au><au>Williams, M.</au><au>Wolfs, J.D.</au><au>Wright, C.J.</au><au>Xia, Q.</au><au>Xiang, X.</au><au>Yin, J.</au><aucorp>Univ. of Rochester, NY (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The data acquisition system of the LZ dark matter detector: FADR</atitle><jtitle>Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment</jtitle><date>2024-11-01</date><risdate>2024</risdate><volume>1068</volume><spage>169712</spage><pages>169712-</pages><artnum>169712</artnum><issn>0168-9002</issn><abstract>The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MHz 32-channel digitizers (DDC-32s). A basic waveform analysis is carried out on the on-board Field Programmable Gate Arrays (FPGAs) to extract information about the observed scintillation and electroluminescence signals. This information is used to determine if the digitized waveforms should be preserved for offline analysis.
The system is designed around the Kintex-7 FPGA. In addition to digitizing the PMT signals and providing basic event selection in real time, the flexibility provided by the use of FPGAs allows us to monitor the performance of the detector and the DAQ in parallel to normal data acquisition.
The hardware and software/firmware of this FPGA-based Architecture for Data acquisition and Realtime monitoring (FADR) are discussed and performance measurements are described.</abstract><cop>United States</cop><pub>Elsevier B.V</pub><doi>10.1016/j.nima.2024.169712</doi><orcidid>https://orcid.org/0000-0001-8693-1196</orcidid><orcidid>https://orcid.org/0000000186931196</orcidid><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, 2024-11, Vol.1068, p.169712, Article 169712 |
issn | 0168-9002 |
language | eng |
recordid | cdi_osti_scitechconnect_2478251 |
source | Elsevier ScienceDirect Journals |
subjects | Dark matter Data acquisition Firmware FPGA |
title | The data acquisition system of the LZ dark matter detector: FADR |
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