Record link: 
http://hdl.handle.net/20.500.12708/140641
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Title: 
A synchronization method for the multi-channel silicon telescope
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Citation: 
Žugec, P., Barbagallo, M., Andrzejewski, J., Perkowski, J., Colonna, N., Bosnar, D., Gawlik, A., Sabate-Gilarte, M., Bacak, M., Mingrone, F., & Chiaveri, E. (2020). A synchronization method for the multi-channel silicon telescope. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 983(164606), 164606. https://doi.org/10.1016/j.nima.2020.164606
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Publisher DOI: 
10.1016/j.nima.2020.164606
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Publication Type: 
Article - Original Research Article
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Language: 
English
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Authors: 
Žugec, Petar 
Barbagallo, Massimo 
Andrzejewski, Jozef 
Perkowski, Jaroslaw 
Colonna, N. 
Bosnar, Damir 
Gawlik, Aleksandra 
Sabate-Gilarte, Marta 
Bacak, Michael 
Mingrone, Federica 
Chiaveri, Enrico 
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Organisational Unit: 
E141-04 - Forschungsbereich Neutron- and Quantum Physics 
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Journal: 
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 
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ISSN: 
0168-9002
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Date (published): 
2020
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Number of Pages: 
7
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Publisher: 
ELSEVIER
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Peer reviewed: 
Yes
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Keywords: 
Instrumentation; Nuclear and High Energy Physics; Silicon telescope; Neutron time of flight; n_TOF facility; Multi-channel synchronization
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Abstract: 
A simple method is presented for the simultaneous off-line synchronization of the digitally recorded data-streams from a multi-channel silicon telescope. The method is based both on the synchronization between the separate pairs of silicon strips and on the synchronization relative to an external timing device. Though only a reduced subset of these constraints is necessary in ideal circumstances, it is shown that this minimal set of conditions may not be sufficient for adequate synchronization in all cases. All available sources of information are therefore considered, in order to constrain the final synchronization as well as possible.
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Research Areas: 
Sensor Systems: 33%
Materials Characterization: 34%
Modelling and Simulation: 33%
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Science Branch: 
Physik, Astronomie
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