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Signal Processing to Reduce Dark Noise Impact in Precision Timing

We introduce a technique to mitigate the effects of low frequency noise on precision timing.The example of Dark Count Noise Rate (DCR) in Silicon Photomultipliers (SiPMs) is emphasized.This technique exploits the correlation between time shifts onthe leading edge of a signal and the residual slope o...

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Autor principal: White, Sebastian
Lenguaje:eng
Publicado: 2023
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1748-0221/18/07/P07051
http://cds.cern.ch/record/2848495
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author White, Sebastian
author_facet White, Sebastian
author_sort White, Sebastian
collection CERN
description We introduce a technique to mitigate the effects of low frequency noise on precision timing.The example of Dark Count Noise Rate (DCR) in Silicon Photomultipliers (SiPMs) is emphasized.This technique exploits the correlation between time shifts onthe leading edge of a signal and the residual slope of the baseline (due to noise) which remainsafter baseline subtraction.In fast timing applications (such as for Time-of-flight particle ID) the signal arrival time is typically captured on the signal leading edge.The signal risetime is often fixed by the physics of the sensor and input circuit. Then accurate pulse timing can be achieved by correcting a leading edge threshold time (depending on a slope proportional to both the Amplitude and the risetime) to a “constant fraction” time.This compensation for time walk due to amplitude fluctuations breaks down once we introduce interference from low frequency noise on the leading edge. In this paper we demonstrate that an additional measurement of the slope at threshold can be used to correct for this noise jitter.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2023
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spelling cern-28484952023-08-11T04:19:32Zdoi:10.1088/1748-0221/18/07/P07051http://cds.cern.ch/record/2848495engWhite, SebastianSignal Processing to Reduce Dark Noise Impact in Precision Timinghep-exParticle Physics - Experimentphysics.ins-detDetectors and Experimental TechniquesWe introduce a technique to mitigate the effects of low frequency noise on precision timing.The example of Dark Count Noise Rate (DCR) in Silicon Photomultipliers (SiPMs) is emphasized.This technique exploits the correlation between time shifts onthe leading edge of a signal and the residual slope of the baseline (due to noise) which remainsafter baseline subtraction.In fast timing applications (such as for Time-of-flight particle ID) the signal arrival time is typically captured on the signal leading edge.The signal risetime is often fixed by the physics of the sensor and input circuit. Then accurate pulse timing can be achieved by correcting a leading edge threshold time (depending on a slope proportional to both the Amplitude and the risetime) to a “constant fraction” time.This compensation for time walk due to amplitude fluctuations breaks down once we introduce interference from low frequency noise on the leading edge. In this paper we demonstrate that an additional measurement of the slope at threshold can be used to correct for this noise jitter.We introduce a technique to mitigate the effects of low frequency noise on precision timing. The example of Dark Count Noise Rate (DCR) in Silicon Photomultipliers (SiPMs) is emphasized. This technique exploits the correlation between time shifts on the leading edge of a signal and the residual slope of the baseline (due to noise) which remains after baseline subtraction. In fast timing applications (such as for Time-of-flight particle ID) the signal arrival time is typically captured on the signal leading edge. The signal risetime is often fixed by the physics of the sensor and input circuit. Then accurate pulse timing can be achieved by correcting a leading edge threshold time (depending on a slope proportional to both the Amplitude and the risetime) to a ``constant fraction" time. This compensation for time walk due to amplitude fluctuations breaks down once we introduce interference from low frequency noise on the leading edge. In this paper we demonstrate that an additional measurement of the slope at threshold can be used to correct for this noise jitter.arXiv:2302.02970FERMILAB-CONF-23-042-CMS-Voai:cds.cern.ch:28484952023-02-06
spellingShingle hep-ex
Particle Physics - Experiment
physics.ins-det
Detectors and Experimental Techniques
White, Sebastian
Signal Processing to Reduce Dark Noise Impact in Precision Timing
title Signal Processing to Reduce Dark Noise Impact in Precision Timing
title_full Signal Processing to Reduce Dark Noise Impact in Precision Timing
title_fullStr Signal Processing to Reduce Dark Noise Impact in Precision Timing
title_full_unstemmed Signal Processing to Reduce Dark Noise Impact in Precision Timing
title_short Signal Processing to Reduce Dark Noise Impact in Precision Timing
title_sort signal processing to reduce dark noise impact in precision timing
topic hep-ex
Particle Physics - Experiment
physics.ins-det
Detectors and Experimental Techniques
url https://dx.doi.org/10.1088/1748-0221/18/07/P07051
http://cds.cern.ch/record/2848495
work_keys_str_mv AT whitesebastian signalprocessingtoreducedarknoiseimpactinprecisiontiming