000576676 001__ 576676
000576676 005__ 20231022003124.0
000576676 0247_ $$2INSPIRETeX$$aBradascio:2023lwj
000576676 0247_ $$2inspire$$ainspire:2628530
000576676 0247_ $$2arXiv$$aarXiv:2301.13828
000576676 0247_ $$2altmetric$$aaltmetric:142002534
000576676 037__ $$aPUBDB-2023-00869
000576676 041__ $$aEnglish
000576676 082__ $$a530
000576676 088__ $$2arXiv$$aarXiv:2301.13828
000576676 1001_ $$0P:(DE-H253)PIP1022296$$aBradascio, Federica$$b0$$eCorresponding author$$udesy
000576676 245__ $$aThe NectarCAM Timing System
000576676 260__ $$c2022
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000576676 500__ $$a8 pages, 13 figures
000576676 520__ $$aNectarCAM 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.
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000576676 588__ $$aDataset connected to INSPIRE
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000576676 650_7 $$2INSPIRE$$aobservatory
000576676 650_7 $$2INSPIRE$$alaser
000576676 650_7 $$2INSPIRE$$abackground
000576676 650_7 $$2INSPIRE$$aphotomultiplier
000576676 650_7 $$2INSPIRE$$ashowers
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000576676 650_7 $$2INSPIRE$$aphoton
000576676 650_7 $$2INSPIRE$$adata acquisition
000576676 650_7 $$2INSPIRE$$asite
000576676 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000576676 650_7 $$2INSPIRE$$anoise
000576676 650_7 $$2INSPIRE$$agamma ray
000576676 650_7 $$2INSPIRE$$aperformance
000576676 650_7 $$2INSPIRE$$aCherenkov
000576676 650_7 $$2INSPIRE$$acosmic radiation
000576676 650_7 $$2INSPIRE$$apixel
000576676 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000576676 7001_ $$0H.Rueda.Ricarte.1$$aRueda, H.$$b1
000576676 7001_ $$0J.A.Barrio.1$$aBarrio, J. A.$$b2
000576676 7001_ $$0J.Biteau.1$$aBiteau, J.$$b3
000576676 7001_ $$aBrun, F.$$b4
000576676 7001_ $$0C.Champion.2$$aChampion, C.$$b5
000576676 7001_ $$0J.F.Glicenstein.1$$aGlicenstein, J-F.$$b6
000576676 7001_ $$aHoffmann, D.$$b7
000576676 7001_ $$0P.Jean.8$$aJean, P.$$b8
000576676 7001_ $$0J.P.Lenain.1$$aLenain, J. P.$$b9
000576676 7001_ $$0F.Louis.1$$aLouis, F.$$b10
000576676 7001_ $$aPerez, A.$$b11
000576676 7001_ $$0M.Punch.1$$aPunch, M.$$b12
000576676 7001_ $$0P.Sizun.1$$aSizun, P.$$b13
000576676 7001_ $$0P:(DE-H253)PIP1003716$$aSulanke, K.-H.$$b14
000576676 7001_ $$0L.A.Tejedor.4$$aTejedor, L. A.$$b15
000576676 7001_ $$0B.Vallage.1$$aVallage, B.$$b16
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