中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A calibration of wfcta prototype telescopes using n-2 laser

文献类型:期刊论文

作者Liu, J. L.1; Zhu, F. R.2; Jia, H. Y.2; Bai, Y. X.3; Cao, Z.3; Chen, M. J.3; Chen, S. Z.3; Feng, S. H.3; Gao, B.3; Gu, M. H.3
刊名Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment
出版日期2018
卷号877页码:278-287
关键词Detector calibration Effective area Light flux Uncertainty
ISSN号0168-9002
DOI10.1016/j.nima.2017.09.041
通讯作者Liu, j. l.(liujiali2017@126.com) ; Zhang, y.(zhangyong@ihep.ac.cn)
英文摘要An end-to-end calibration method, which is different from the traditional way, has been employed in wfcta prototype experiment based on n-2 laser. as we known, the calculation of the expected and the observed light fluxes at the front of the aperture of the telescope are crucial in the such method. to calculate predicted light flux accurately, the propagation and scattering of photons in the atmosphere have been considered in detail. in order to get the detector effective areas, which will be used in the transformation of adc signals to the observed light flux, a ray trace procedure, considering all details of detector response, has been performed for all incident direction of photons in field of view of the detector. by matching the observed and expected light flux at the entrance of the telescope, the overall calibration gains of two telescopes can be obtained. during the test run of the calibration, a overall calibration gain around g = 0.38 adc counts/photon and g = 0.36 adc counts/photon for wfct01 and wfct02 are given, respectively. furthermore, in view of all uncertainty sources, systematic uncertainties for the calibration have also been estimated. they are around the level of (-7.3%, + 7.8%). the calibration results achieved by end-to-end method and the traditional way are in consistent at the level of 10%, which is within the range of uncertainties. since the end-to-end and traditional calibration methods have their own advantages, the performance of the combination of these two calibration methods has also been discussed in the end. (c) 2017 elsevier b.v. all rights reserved.
WOS关键词PROJECT ; LHAASO ; YBJ
WOS研究方向Instruments & Instrumentation ; Nuclear Science & Technology ; Physics
WOS类目Instruments & Instrumentation ; Nuclear Science & Technology ; Physics, Nuclear ; Physics, Particles & Fields
语种英语
WOS记录号WOS:000415128000035
出版者ELSEVIER SCIENCE BV
URI标识http://www.irgrid.ac.cn/handle/1471x/2176884
专题高能物理研究所
通讯作者Liu, J. L.; Zhang, Y.
作者单位1.Kunming Univ, Phys Dept, Kunming 650214, Yunnan, Peoples R China
2.Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
4.Normal Coll Fuyang, Phys Dept, Fuyang 236037, Peoples R China
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Liu, J. L.,Zhu, F. R.,Jia, H. Y.,et al. A calibration of wfcta prototype telescopes using n-2 laser[J]. Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment,2018,877:278-287.
APA Liu, J. L..,Zhu, F. R..,Jia, H. Y..,Bai, Y. X..,Cao, Z..,...&Zuo, X..(2018).A calibration of wfcta prototype telescopes using n-2 laser.Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment,877,278-287.
MLA Liu, J. L.,et al."A calibration of wfcta prototype telescopes using n-2 laser".Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment 877(2018):278-287.

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