001     576676
005     20231022003124.0
024 7 _ |a Bradascio:2023lwj
|2 INSPIRETeX
024 7 _ |a inspire:2628530
|2 inspire
024 7 _ |a arXiv:2301.13828
|2 arXiv
024 7 _ |a altmetric:142002534
|2 altmetric
037 _ _ |a PUBDB-2023-00869
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2301.13828
|2 arXiv
100 1 _ |a Bradascio, Federica
|0 P:(DE-H253)PIP1022296
|b 0
|e Corresponding author
|u desy
245 _ _ |a The NectarCAM Timing System
260 _ _ |c 2022
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1697797745_1825962
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a 8 pages, 13 figures
520 _ _ |a NectarCAM is a Cherenkov camera which is going to equip the Medium-Sized Telescopes (MST) of the northern site of the Cherenkov Telescope Array Observatory (CTAO). NectarCAM is equipped with 265 modules, each consisting of 7 photo-multiplier tubes (PMTs), a Front-End Board and a local camera trigger system used for data acquisition. This paper addresses the timing performances of NectarCAM which are crucial to reduce the noise in shower images and improve image cleaning as well as to discriminate between gamma-ray photons and cosmic-ray background and finally to allow coincidence identification with neighbouring telescopes for stereoscopic operations. Verification tests of the system have been performed in a dark room using various light sources to illuminate the first NectarCAM unit. The resulting timing precision and accuracy of the trigger arrival relative to a laser source, of individual and multiple pixel signals have been studied and are shown to comply to CTAO requirements.
536 _ _ |a 899 - ohne Topic (POF4-899)
|0 G:(DE-HGF)POF4-899
|c POF4-899
|f POF IV
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a trigger
|2 INSPIRE
650 _ 7 |a observatory
|2 INSPIRE
650 _ 7 |a laser
|2 INSPIRE
650 _ 7 |a background
|2 INSPIRE
650 _ 7 |a photomultiplier
|2 INSPIRE
650 _ 7 |a showers
|2 INSPIRE
650 _ 7 |a tube
|2 INSPIRE
650 _ 7 |a photon
|2 INSPIRE
650 _ 7 |a data acquisition
|2 INSPIRE
650 _ 7 |a site
|2 INSPIRE
650 _ 7 |a Cherenkov Telescope Array
|2 INSPIRE
650 _ 7 |a noise
|2 INSPIRE
650 _ 7 |a gamma ray
|2 INSPIRE
650 _ 7 |a performance
|2 INSPIRE
650 _ 7 |a Cherenkov
|2 INSPIRE
650 _ 7 |a cosmic radiation
|2 INSPIRE
650 _ 7 |a pixel
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Rueda, H.
|0 H.Rueda.Ricarte.1
|b 1
700 1 _ |a Barrio, J. A.
|0 J.A.Barrio.1
|b 2
700 1 _ |a Biteau, J.
|0 J.Biteau.1
|b 3
700 1 _ |a Brun, F.
|b 4
700 1 _ |a Champion, C.
|0 C.Champion.2
|b 5
700 1 _ |a Glicenstein, J-F.
|0 J.F.Glicenstein.1
|b 6
700 1 _ |a Hoffmann, D.
|b 7
700 1 _ |a Jean, P.
|0 P.Jean.8
|b 8
700 1 _ |a Lenain, J. P.
|0 J.P.Lenain.1
|b 9
700 1 _ |a Louis, F.
|0 F.Louis.1
|b 10
700 1 _ |a Perez, A.
|b 11
700 1 _ |a Punch, M.
|0 M.Punch.1
|b 12
700 1 _ |a Sizun, P.
|0 P.Sizun.1
|b 13
700 1 _ |a Sulanke, K.-H.
|0 P:(DE-H253)PIP1003716
|b 14
700 1 _ |a Tejedor, L. A.
|0 L.A.Tejedor.4
|b 15
700 1 _ |a Vallage, B.
|0 B.Vallage.1
|b 16
856 4 _ |u https://bib-pubdb1.desy.de/record/576676/files/2302.07611v2.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/576676/files/2302.07611v2.pdf?subformat=pdfa
|x pdfa
|y Restricted
909 C O |o oai:bib-pubdb1.desy.de:576676
|p VDB
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 0
|6 P:(DE-H253)PIP1022296
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 14
|6 P:(DE-H253)PIP1003716
913 1 _ |a DE-HGF
|b Programmungebundene Forschung
|l ohne Programm
|1 G:(DE-HGF)POF4-890
|0 G:(DE-HGF)POF4-899
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-800
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|v ohne Topic
|x 0
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
920 1 _ |0 I:(DE-H253)Z_EL-20210408
|k Z_EL
|l Elektronik
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)Z_EL-20210408
980 _ _ |a UNRESTRICTED


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