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Featured researches published by X. X. Li.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2018

Internal alignment and position resolution of the silicon tracker of DAMPE determined with orbit data

A. Tykhonov; G. Ambrosi; R. Asfandiyarov; P. Azzarello; P. Bernardini; B. Bertucci; A. Bolognini; F. Cadoux; A. D’Amone; A. De Benedittis; I. De Mitri; M. Di Santo; Yuhui Dong; M. Duranti; D. D’Urso; R.R. Fan; P. Fusco; Valentina Gallo; M. Gao; F. Gargano; S. Garrappa; Keyun Gong; M. Ionica; D. La Marra; Shi-Jun Lei; X. X. Li; F. Loparco; G. Marsella; M. N. Mazziotta; W.X. Peng

Abstract The DArk Matter Particle Explorer (DAMPE) is a space-borne particle detector designed to probe electrons and gamma-rays in the few GeV to 10 TeV energy range, as well as cosmic-ray proton and nuclei components between 10 GeV and 100 TeV. The silicon–tungsten tracker–converter is a crucial component of DAMPE. It allows the direction of incoming photons converting into electron–positron pairs to be estimated, and the trajectory and charge (Z) of cosmic-ray particles to be identified. It consists of 768 silicon micro-strip sensors assembled in 6 double layers with a total active area of 6.6 m 2 . Silicon planes are interleaved with three layers of tungsten plates, resulting in about one radiation length of material in the tracker. Internal alignment parameters of the tracker have been determined on orbit, with non-showering protons and helium nuclei. We describe the alignment procedure and present the position resolution and alignment stability measurements.


The Astrophysical Journal | 2013

TeV gamma-ray survey of the northern sky using the ARGO-YBJ detector

B. Bartoli; P. Bernardini; X. J. Bi; I. Bolognino; P. Branchini; A. Budano; A. K. Calabrese Melcarne; P. Camarri; Z. Cao; R. Cardarelli; S. Catalanotti; Songzhan Chen; T. L. Chen; Y. B. Chen; P. Creti; S. W. Cui; B. Z. Dai; A. D'Amone; Danzengluobu; I. De Mitri; B. D'Ettorre Piazzoli; T. Di Girolamo; X. H. Ding; G. Di Sciascio; C. F. Feng; Zhaoyang Feng; Z. Y. Feng; Q. B. Gou; Y. Q. Guo; H. H. He


The Astrophysical Journal | 2016

SYSTEMATIC NON-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu*

G. Zhao; Lyudmila Mashonkina; H. L. Yan; S. Alexeeva; Chiaki Kobayashi; Yu. V. Pakhomov; J. R. Shi; T. Sitnova; K. F. Tan; H. W. Zhang; Jianchao Zhang; Zhimin Zhou; Michael Bolte; Yanting Chen; X. X. Li; Fan Liu; Meng Zhai


Chinese Physics C | 2014

Energy spectrum of cosmic protons and helium nuclei by a hybrid measurement at 4300 m a.s.l.

B. Bartoli; P. Bernardini; X. J. Bi; I. Bolognino; P. Branchini; A. Budano; A. K. Calabrese Melcarne; P. Camarri; Z. Cao; R. Cardarelli; S. Catalanotti; S. Chen; T. L. Chen; P. Creti; S. W. Cui; B. Z. Dai; A. D'Amone; Danzengluobu; I. De Mitri; B. D'Ettorre Piazzoli; T. Di Girolamo; G. Di Sciascio; C. F. Feng; Zhaoyang Feng; Z. Y. Feng; Q. B. Gou; Y. Q. Guo; H. H. He; Haibing Hu; Hongbo Hu

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I. De Mitri

Istituto Nazionale di Fisica Nucleare

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P. Bernardini

Istituto Nazionale di Fisica Nucleare

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A. Budano

Istituto Nazionale di Fisica Nucleare

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A. D'Amone

Istituto Nazionale di Fisica Nucleare

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A. K. Calabrese Melcarne

Istituto Nazionale di Fisica Nucleare

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B. Bartoli

Istituto Nazionale di Fisica Nucleare

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B. D'Ettorre Piazzoli

Istituto Nazionale di Fisica Nucleare

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G. Di Sciascio

Istituto Nazionale di Fisica Nucleare

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P. Branchini

Istituto Nazionale di Fisica Nucleare

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