6533b821fe1ef96bd127c1fe

RESEARCH PRODUCT

Software Timing Calibration of the ARGO-YBJ Detector

A. CappaF. R. ZhuL. PerroneM. PanareoP. ZhangC. Y. WuP. SalviniA. F. YuanL. ZhangQ. Q. ZhuX. R. MengY.g. WangN. ChengP. PistilliP. PistilliC. StanescuZhaoyang FengX. X. ZhouS. MastroianniS. MastroianniS. CatalanottiH.t. YangPiero VallaniaC. VigoritoC. VigoritoL. SaggeseX. C. YangP. GaleottiP. GaleottiB. D'ettorre PiazzoliJ. K. K. LiuH. J. LiH. R. WuA. BudanoZhengguo CaoH. Y. JiaM. IacovacciM. ZhaR. GarganaLabacirenC. BacciC. BacciC. CattaneoT. Di GirolamoM. DattoliM. DattoliX. Y. GaoL. XueP. CelioP. CelioG.c. YuHaoqi LuZhaxisangzhuI. JamesI. JamesQ. HuangG. Di SciascioG. CusumanoC. PinoF. ShiDanzengluobuP. CretiC.c. NingM. De VincenziM. De VincenziC. LiuSergio CavaliereLuciano NicastroA. K. Calabrese MelcarneC. FerrignoA. SegretoR. CardarelliY. H. ZhangG. MarsellaB. LibertiG. MancarellaB. BartoliP. CamarriE. RossiX. Y. ZhangH. W. WangS. W. CuiZhenyong FengHuihai HeS. VernettoF. GaleazziX. D. ShengPaolo BernardiniHongbo HuA. SurdoC. F. FengR. SantonicoP. R. ShenG. AielliZhang JingzheBingwei XuSeverino Angelo Maria BussinoSeverino Angelo Maria BussinoQ. B. GouJ. Y. LiI. De MitriL. PalummoH. M. ZhangQ. Y. YangG. D'alí StaitiG. D'alí StaitiG. ZizziS. M. MariS. M. MariJ. MuX. J. BiS. Z. ChenB. Z. DaiF. RuggieriP. BranchiniX. B. QuX. H. DingY. H. TanG. LiguoriG. LiguoriHaibing HuC. BleveD. Martello

subject

PhysicsPixelCalibration (statistics)business.industryPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorSettore FIS/01 - Fisica SperimentaleComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsAstronomia gammaGamma Astronomy Timing Calibration Extensive Air ShowersSciami estesiCalibrazione temporaleOpticsSoftwareRaggi cosmiciSettore FIS/05 - Astronomia e AstrofisicaAngular resolutionbusinessArgoRemote sensing

description

The ARGO-YBJ experiment is mainly devoted to search for astronomical gamma sources. The arrival direction of air showers is reconstructed thanks to the times measured by the pixels of the detector. Therefore, the timing calibration of the detector pixels is crucial in order to get the best angular resolution and pointing accuracy. Because of the large number of pixels a hardware timing calibration is practically impossible. Therefore an off-line software calibration has been adopted. Here, the details of the procedure and the results are presented. (C) 2008 Elsevier B.V. All rights reserved.

https://hdl.handle.net/11587/106235