Jingjing Zang
Chinese Academy of Sciences
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Publication
Featured researches published by Jingjing Zang.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2017
Chuan Yue; Jingjing Zang; Tiekuang Dong; Xiang Li; Zhiyong Zhang; S. Zimmer; Wei Jiang; Yunlong Zhang; Daming Wei
Abstract DAMPE is a space-based mission designed as a high energy particle detector measuring cosmic-rays and γ -rays which was successfully launched on Dec.17, 2015. The BGO electromagnetic calorimeter is one of the key sub-detectors of DAMPE for energy measurement of electromagnetic showers produced by e ± / γ . Due to energy loss in dead material and energy leakage outside the calorimeter, the deposited energy in BGO underestimates the primary energy of incident e ± / γ . In this paper, based on detailed MC simulations, a parameterized energy correction method using the lateral and longitudinal information of electromagnetic showers has been studied and verified with data of electron beam test at CERN. The measurements of energy linearity and resolution are significant improved by applying this correction method for electromagnetic showers.
Research in Astronomy and Astrophysics | 2018
Zun-Lei Xu; Kai-Kai Duan; Zhao-Qiang Shen; Shi-Jun Lei; Tiekuang Dong; F. Gargano; Simone Garrappa; Dongya Guo; Wei Jiang; Xiang Li; Yun-Feng Liang; Mario Nicola Mazziotta; M.M. Salinas; Meng Su; Valerio Vagelli; Qiang Yuan; Chuan Yue; Jingjing Zang; Yapeng Zhang; Yunlong Zhang; S. Zimmer
The DArk Matter Particle Explorer (DAMPE), also known as Wukong in China, launched on December 17, 2015, is a new high energy cosmic ray and {\gamma}-ray satellite-borne observatory in space. One of the main scientific goals of DAMPE is to observe GeV-TeV high energy {\gamma}-rays with accurate energy, angular, and time resolution, to indirectly search for dark matter particles and for the study of high energy astrophysics. Due to the comparatively higher fluxes of charged cosmic rays with respect to {\gamma}-rays, it is challenging to identify {\gamma}-rays with sufficiently high efficiency minimizing the amount of charged cosmic ray contamination. In this work we present a method to identify {\gamma}-rays in DAMPE data based on Monte Carlo simulations, using the powerful electromagnetic/hadronic shower discrimination provided by the calorimeter and the veto detection of charged particles provided by the plastic scintillation detector. Monte Carlo simulations show that after this selection the number of electrons and protons that contaminate the selected {\gamma}-ray events at
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Jingjing Zang; Chuan Yue; Xiang Li
\sim10
Chinese Physics C | 2017
Chi Wang; Dong Liu; Yifeng Wei; Zhiyong Zhang; Yunlong Zhang; Xiaolian Wang; Z. Xu; G. S. Huang; A. Tykhonov; Xin Wu; Jingjing Zang; Yang Liu; Wei Jiang; Sicheng Wen; Jian Wu; Jin Chang
GeV amounts to less than 1% of the selected sample. Finally, we use flight data to verify the effectiveness of the method by highlighting known {\gamma}-ray sources in the sky and by reconstructing preliminary light curves of the Geminga pulsar.
Astroparticle Physics | 2019
Tiekuang Dong; Yapeng Zhang; Peng-Xiong Ma; Yongjie Zhang; P. Bernardini; Meng Ding; Dongya Guo; Shi-Jun Lei; Xiang Li; Ivan De Mitri; W.X. Peng; Rui Qiao; Margherita Di Santo; Zhi-Yu Sun; Antonio Surdo; Z.M. Wang; Jian Wu; Zun-Lei Xu; Y. Yu; Qiang Yuan; Chuan Yue; Jingjing Zang; Yunlong Zhang
In this paper, we developed a method to determine absolute energy scale of DAMPE via measuring geomagnetic cutoff on cosmic ray electron and positron spectrum. The rigidity cutoff on cosmic ray electron and positron was calculated using IGRF-12 model and cosmic ray particle trajectory tracing code developed by Smart and Shea. Then we also measured cosmic ray electron and positron spectrum in MacIlwain L bin [1,1.14] based on over 425 days flight data of DAMPE. By directly comparing calculated geomagnetic cutoff with DAMPE measured result, we provide an estimation on absolute energy scale of DAMPE
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Chuan Yue; Jingjing Zang; Tiekuang Dong; A. Surdo; Stefania Vitillo
1.25\%
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Wei Jiang; Xiang Li; Jingjing Zang; Chuan Yue; Yuan-Peng Wang
higher than expected at about 13GeV energy with uncertainty about
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Zun-Lei Xu; Xiang Li; Jingjing Zang; Wei Jiang; Yao Li
\pm1.75\%(stat)\pm1.34\%(sys)
Archive | 2017
Yuan-Peng Wang; Sicheng Wen; Wei Jiang; Chuan Yue; Zhiyong Zhang; Yifeng Wei; Yun-LongZhang; Jingjing Zang; Jian Wu
.
Chinese Physics C | 2017
Yuan-Peng Wang; Sicheng Wen; Wei Jiang; Chuan Yue; Zhiyong Zhang; Yifeng Wei; Yunlong Zhang; Jingjing Zang; Jian Wu
A software framework has been developed for the DArk Matter Particle Explorer (DAMPE) mission, a satellite based experiment. The software framework of DAMPE is mainly written in C++, while the application under this framework is steered in Python script. The framework is comprised of four principal parts: event data module which contains all reconstruction and simulation information based on ROOT input/output (I/O) streaming; a collection of processing models which are used to process each event data, called as algorithms; service module, a series of common tools which provide general functionalities like data communication between algorithms; and event filters. This article presents an overview of the DAMPE offline software framework, and the major architecture design choices during the development. The whole system has been applied to DAMPE data analysis successfully, based on which some results from simulation and beam test experiments are also shown in this article.