Artículos de revistas: "DAMPE"

1

Fowlie, Andrew. "DAMPE squib? Significance of the 1.4 TeV DAMPE excess". Physics Letters B 780 (mayo de 2018): 181–84. http://dx.doi.org/10.1016/j.physletb.2018.03.006.

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2

Stolpovskiy, M., X. Wu, A. Tykhonov, M. Deliyergiyev, C. Perrina, M. Muñoz Salinas, D. Droz, A. Ruina y E. Catanzani. "Machine learning-based method of calorimeter saturation correction for helium flux analysis with DAMPE experiment". Journal of Instrumentation 17, n.º 06 (1 de junio de 2022): P06031. http://dx.doi.org/10.1088/1748-0221/17/06/p06031.

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Abstract DAMPE is a space-borne experiment for the measurement of the cosmic-ray fluxes at energies up to around 100 TeV per nucleon. At energies above several tens of TeV, the electronics of DAMPE calorimeter would saturate, leaving certain bars with no energy recorded. In the present work we discuss the application of machine learning techniques for the treatment of DAMPE data, to compensate the calorimeter energy lost by saturation.

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3

Azzarello, P., G. Ambrosi, R. Asfandiyarov, P. Bernardini, B. Bertucci, A. Bolognini, F. Cadoux et al. "The DAMPE silicon–tungsten tracker". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 831 (septiembre de 2016): 378–84. http://dx.doi.org/10.1016/j.nima.2016.02.077.

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4

Wang, S. X., J. J. Zang, W. Jiang, S. J. Lei, C. N. Luo, Z. L. Xu y J. Chang. "A Study on Monte Carlo Simulation of the Radiation Environment above GeV at the DAMPE Orbit". Research in Astronomy and Astrophysics 22, n.º 4 (17 de marzo de 2022): 045011. http://dx.doi.org/10.1088/1674-4527/ac550e.

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Abstract The Dark Matter Particle Explorer (DAMPE) has been undergoing a stable on-orbit operation for more than 6 yr and acquired observations of over 11 billion events. A better understanding of the overall radiation environment of the DAMPE orbit is crucial for both simulation data production and flight data analysis. In this work, we study the radiation environment at low Earth orbit and develop a simulation software package using the framework of ATMNC3, in which state-of-the-art full 3D models of the Earth’s atmospheric and magnetic-field configurations are integrated. We consider in our Monte Carlo procedure event-by-event propagation of cosmic rays in the geomagnetic field and their interaction with the Earth’s atmosphere, focusing on the particles above GeV that are able to trigger the DAMPE data acquisition system. We compare the simulation results with the cosmic-ray electron and positron (CRE) flux measurements made by DAMPE. The overall agreement on both the spectral and angular distribution of the CRE flux demonstrates that our simulation is well established. Our software package could be of more general usage for simulation of the radiation environment of low Earth orbit at various altitudes.

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5

Bernardini, Paolo. "Main scientific results of the DAMPE mission". EPJ Web of Conferences 209 (2019): 01048. http://dx.doi.org/10.1051/epjconf/201920901048.

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DAMPE (DArk Matter Particle Explorer) is a satellite-born experiment, resulting from the collaboration of Chinese, Italian, and Swiss institutions. Since December 2015, DAMPE flights at the altitude of 500 km and collects data smoothly. The detector is made of four sub-detectors: top layers of plastic scintillators, a silicon-tungsten tracker, a BGO calorimeter (32 radiation lengths), and a bottom boron-doped scintillator to detect delayed neutrons. The main goal of the experiment is the search for indirect signals of Dark Matter in the electron and photon spectra with energies up to 10 TeV. Furthermore DAMPE studies cosmic charged and gamma radiation. The calorimeter depth and the large acceptance allow to measure cosmic ray fluxes in the range from 20 GeV up to hundreds of TeV. An overview of the latest results about light component (p+He) of charged cosmic rays, gamma astronomy and electron and positron spectrum will be presented.

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6

Yu, Yuhong, Zhiyu Sun, Hong Su, Yaqing Yang, Jie Liu, Jie Kong, Guoqing Xiao et al. "The plastic scintillator detector for DAMPE". Astroparticle Physics 94 (septiembre de 2017): 1–10. http://dx.doi.org/10.1016/j.astropartphys.2017.06.004.

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7

Lu, Tong-suo, Shi-jun Lei, Jing-jing Zang, Jin Chang y Jian Wu. "Study of Track Reconstruction for DAMPE". Chinese Astronomy and Astrophysics 41, n.º 3 (julio de 2017): 455–70. http://dx.doi.org/10.1016/j.chinastron.2017.08.012.

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8

Wang, Chi, Dong Liu, Yifeng Wei, Zhiyong Zhang, Yunlong Zhang, Xiaolian Wang, Zizong Xu et al. "Offline software for the DAMPE experiment". Chinese Physics C 41, n.º 10 (28 de septiembre de 2017): 106201. http://dx.doi.org/10.1088/1674-1137/41/10/106201.

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9

Dai, Hao-Ting, Jing-Jing Zang, Ying Wang, Chuan-Ning Luo, Yun-Long Zhang, Zhi-Yong Zhang, Yi-Feng Wei et al. "Method of Separating Cosmic-Ray Positrons from Electrons in the DAMPE Experiment". Research in Astronomy and Astrophysics 22, n.º 3 (18 de febrero de 2022): 035012. http://dx.doi.org/10.1088/1674-4527/ac47a8.

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Abstract A method of identifying positron/electron species from the cosmic rays was studied in the DArk Matter Particle Explorer (DAMPE) experiment. As there is no onboard magnet on the satellite, the different features imposed by the geomagnetic field on these two species were exploited for the particle identification. Application of this method to the simulation of on-orbit electrons/positrons/protons and the real flight data proves that separately measuring the CR positrons/electrons with DAMPE is feasible, though limited by the field of view for the present observation data. Further analysis on the positron flux with this method can be expected in the future.

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10

Mitri, I. De, A. Parenti y L. Silveri. "Selected Results from the DAMPE Space Mission". Physics of Atomic Nuclei 84, n.º 6 (noviembre de 2021): 947–55. http://dx.doi.org/10.1134/s106377882113007x.

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11

Fusco, Piergiorgio. "The DAMPE experiment and its latest results". Journal of Physics: Conference Series 1390 (noviembre de 2019): 012063. http://dx.doi.org/10.1088/1742-6596/1390/1/012063.

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12

De Mitri, Ivan. "The DAMPE experiment: first data from space". EPJ Web of Conferences 136 (2017): 02010. http://dx.doi.org/10.1051/epjconf/201713602010.

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13

De Benedittis, Antonio. "Proton energy spectrum with the DAMPE experiment". EPJ Web of Conferences 209 (2019): 01030. http://dx.doi.org/10.1051/epjconf/201920901030.

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The DAMPE (DArk Matter Particle Explorer) experiment, in orbit since December 17th 2015, is a space mission whose main purpose is the detection of cosmic electrons and photons up to energies of 10 TeV, in order to identify possible evidence of Dark Matter in their spectra. Furthermore it aims to measure the spectra and the elemental composition of the galactic cosmic rays nuclei up to the energy of hundreds of TeV. The proton analysis and the flux with kinetic energy ranging from 50 GeV up to 100 TeV, at the end of two years of data taking, will be presented and discussed.

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14

Bernardini, Paolo. "Main scientific results of the DAMPE mission". Journal of Physics: Conference Series 1181 (febrero de 2019): 012043. http://dx.doi.org/10.1088/1742-6596/1181/1/012043.

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15

Bernardini, Paolo. "First data from the DAMPE space mission". Nuclear and Particle Physics Proceedings 291-293 (octubre de 2017): 59–65. http://dx.doi.org/10.1016/j.nuclphysbps.2017.06.014.

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16

Ming, He, Ma Tao, Chang Jin, Zhang Yan, Huang Yong-yi, Zang Jing-jing, Wu Jian y Dong Tie-kuang. "GEANT4 Simulation of Neutron Detector for DAMPE". Chinese Astronomy and Astrophysics 40, n.º 4 (octubre de 2016): 474–82. http://dx.doi.org/10.1016/j.chinastron.2016.10.002.

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17

Wang, Pei-Long, Yun-Long Zhang, Xiao-Lian Wang y Zi-Zong Xu. "Magnetic shielding for DAMPE electromagnetic calorimeter PMTs". Chinese Physics C 38, n.º 8 (agosto de 2014): 086002. http://dx.doi.org/10.1088/1674-1137/38/8/086002.

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18

Chan, Man Ho y Chak Man Lee. "Origin of the DAMPE 1.4 TeV peak". Monthly Notices of the Royal Astronomical Society: Letters 486, n.º 1 (2 de mayo de 2019): L85—L88. http://dx.doi.org/10.1093/mnrasl/slz062.

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19

Gargano, Fabio. "The DAMPE experiment: 2 year in orbit". Journal of Physics: Conference Series 934 (diciembre de 2017): 012015. http://dx.doi.org/10.1088/1742-6596/934/1/012015.

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20

Belotsky, Konstantin, Airat Kamaletdinov, Maxim Laletin y Maxim Solovyov. "The DAMPE excess and gamma-ray constraints". Physics of the Dark Universe 26 (diciembre de 2019): 100333. http://dx.doi.org/10.1016/j.dark.2019.100333.

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21

Xiang, Yu Hua, Jia Yuan Zhang y Xiao Hui Zhang. "Research of Cold Test in 170t/h Tangentially Fired Boiler". Advanced Materials Research 516-517 (mayo de 2012): 180–86. http://dx.doi.org/10.4028/www.scientific.net/amr.516-517.180.

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The characteristics of the WGZ170/9.8-3 pulverized coal boiler were obtained based on cold test，Including the air velocity distribution in tangential firing boiler and the relation between air distribution with opening of each secondary air dampe，The test results had determined that the baffle of blower at around 40% and two parallel draft fan about 45% were relatively appropriate. and the air distribution and opening of each secondary air dampe and balancing the distribution of primary air and second air along the width direction of the boiler hearth were confirmed through test，and the aerodynamic field inside the boiler was investigated based on the tie-floating test．and good aerodynamic field can be obtained after distributing the primary air and second air reasonably，which guarantee the ignition and stable operation of the boiler．

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22

Alemanno, Francesca. "The DAMPE Space Mission: Status and Main Results". Moscow University Physics Bulletin 77, n.º 2 (abril de 2022): 280–83. http://dx.doi.org/10.3103/s0027134922020060.

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23

Tykhonov, A., G. Ambrosi, R. Asfandiyarov, P. Azzarello, P. Bernardini, B. Bertucci, A. Bolognini et al. "In-flight performance of the DAMPE silicon tracker". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 924 (abril de 2019): 309–15. http://dx.doi.org/10.1016/j.nima.2018.06.036.

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24

Dong, Yi-Fan, Fei Zhang, Rui Qiao, Wen-Xi Peng, Rui-Rui Fan, Ke Gong, Di Wu y Huan-Yu Wang. "DAMPE silicon tracker on-board data compression algorithm". Chinese Physics C 39, n.º 11 (noviembre de 2015): 116202. http://dx.doi.org/10.1088/1674-1137/39/11/116202.

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25

Wu, Li-Bo, Yun-Long Zhang, Zhi-Yong Zhang, Yi-Feng Wei, Si-Cheng Wen, Hao-Ting Dai, Cheng-Ming Liu, Xiao-Lian Wang, Zi-Zong Xu y Guang-Shun Huang. "Energy correction based on fluorescence attenuation of DAMPE". Research in Astronomy and Astrophysics 20, n.º 8 (agosto de 2020): 118. http://dx.doi.org/10.1088/1674-4527/20/8/118.

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26

HU Yiming, CHANG Jin, CHEN Dengyi, LIU Shubin, FENG Changqing y ZHANG Yunlong. "Thermal Design and Validation of DAMPE BGO Calorimeter". Chinese Journal of Space Science 37, n.º 1 (2017): 114. http://dx.doi.org/10.11728/cjss2017.01.114.

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27

Catanzani, E., G. Ambrosi, P. Azzarello, C. Perrina, M. Iónica, A. Tykhonov y X. Wu. "Study of the performances of the DAMPE silicon-tungsten tracker after five years of mission". Journal of Physics: Conference Series 2374, n.º 1 (1 de noviembre de 2022): 012067. http://dx.doi.org/10.1088/1742-6596/2374/1/012067.

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DAMPE (DArk Matter Particle Explorer) is a satellite-based experiment launched in December 2015 and smoothly taking data after five years of mission. The Silicon-Tungsten Tracker (STK) is characterized by 6 double layers of silicon micro-strip detectors, for a total detection area of 7 m2, and three 1 mm thick tungsten plates, placed in the mechanical support structure, aimed to the photon conversion in e± pairs. The STK has a double role: precise reconstruction of the track of charged particles with a spatial resolution around 40 μm for most incident angles of the incoming particles, identification of the charge of the incoming cosmic rays. The STK performances are excellent after five years of continuous operation in space: in this contribution the STK in-orbit calibration and performances during the whole DAMPE mission will be presented.

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28

Okada, Nobuchika y Osamu Seto. "DAMPE excess from decaying right-handed neutrino dark matter". Modern Physics Letters A 33, n.º 27 (2 de septiembre de 2018): 1850157. http://dx.doi.org/10.1142/s0217732318501572.

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The flux of high-energy cosmic-ray electrons plus positrons recently measured by the DArk Matter Particle Explorer (DAMPE) exhibits a tentative peak excess at an energy of around 1.4 TeV. In this paper, we consider the minimal gauged U(1)[Formula: see text] model with a right-handed neutrino (RHN) dark matter (DM) and interpret the DAMPE peak with a late-time decay of the RHN DM into [Formula: see text]. We find that a DM lifetime [Formula: see text] can fit the DAMPE peak with a DM mass [Formula: see text]. This favored lifetime is close to the current bound on it by Fermi-LAT, our decaying RHN DM can be tested, once the measurement of cosmic gamma ray flux is improved. The RHN DM communicates with the Standard Model particles through the U(1)[Formula: see text] gauge boson ([Formula: see text] boson), and its thermal relic abundance is controlled by only three free parameters: [Formula: see text], the U(1)[Formula: see text] gauge coupling [Formula: see text], and the [Formula: see text] boson mass [Formula: see text]. For [Formula: see text], the rest of the parameters are restricted to be [Formula: see text] and [Formula: see text], in order to reproduce the observed DM relic density and to avoid the Landau pole for running [Formula: see text] below the Planck scale. This allowed region will be tested by the search for a [Formula: see text] boson resonance at the future Large Hadron Collider.

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29

Babynets, Nelya. "Death as Poetic Device in John Donne’s The Dampe". IAFOR Journal of Arts & Humanities 7, n.º 1 (6 de junio de 2020): 3–16. http://dx.doi.org/10.22492/ijah.7.1.01.

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30

Tykhonov, A., V. Gallo, X. Wu y S. Zimmer. "Reconstruction software of the silicon tracker of DAMPE mission". Journal of Physics: Conference Series 898 (octubre de 2017): 042031. http://dx.doi.org/10.1088/1742-6596/898/4/042031.

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31

Qiao, Rui, Wen-Xi Peng, G. Ambrosi, R. Asfandiyarov, P. Azzarello, P. Bernardini, B. Bertucci et al. "A charge reconstruction algorithm for DAMPE silicon microstrip detectors". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 935 (agosto de 2019): 24–29. http://dx.doi.org/10.1016/j.nima.2019.04.036.

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32

Zhang, Yongjie, Zhiyu Sun, Yuhong Yu, Jianhua Guo, Fang Fang, Yong Zhou, Zhaoming Wang, Yapeng Zhang y Bitao Hu. "A survey of space radiation damage to DAMPE-PSD". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 971 (agosto de 2020): 164112. http://dx.doi.org/10.1016/j.nima.2020.164112.

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33

Wang, Zhao-Min, Yu-Hong Yu, Zhi-Yu Sun, Ke Yue, Duo Yan, Yong-Jie Zhang, Yong Zhou, Fang Fang, Wen-Xue Huang y Jun-Ling Chen. "Temperature dependence of the plastic scintillator detector for DAMPE". Chinese Physics C 41, n.º 1 (enero de 2017): 016001. http://dx.doi.org/10.1088/1674-1137/41/1/016001.

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34

Parenti, Andrea. "Galactic cosmic rays: latest results from the DAMPE mission". Journal of Physics: Conference Series 2429, n.º 1 (1 de febrero de 2023): 012003. http://dx.doi.org/10.1088/1742-6596/2429/1/012003.

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Abstract The space-based DAMPE (DArk Matter Particle Explorer) particle detector has been taking data for more than 6 years since its successful launch in December 2015. Its main scientific goals include the indirect search of Dark Matter signatures in the cosmic lepton spectra, the study of Galactic Cosmic Rays up to energies of hundreds of TeV and high-energy gamma ray astronomy. This talk will focus on Galactic Cosmic Rays and the measurement of their spectra, fundamental to investigate the mechanisms of acceleration at their sources and propagation through the interstellar medium. The most recent results on Proton and Helium, which revealed new spectral features, will be highlighted. Ongoing analyses regarding the cosmic ray light component, medium and heavy mass nuclei will be discussed alongside studies on the so-called secondary cosmic rays.

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35

Bao, Yiwei, Yang Chen y Siming Liu. "Is PSR J0855−4644 responsible for the 1.4 TeV electron spectral bump hinted by DAMPE?" Monthly Notices of the Royal Astronomical Society 500, n.º 4 (27 de octubre de 2020): 4573–77. http://dx.doi.org/10.1093/mnras/staa3311.

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ABSTRACT DAMPE observation on the cosmic ray electron spectrum hints a narrow excess at ∼1.4 TeV. Although the excess can be ascribed to dark matter particles, pulsars and pulsar wind nebulae are believed to be more natural astrophysical origins: electrons injected from nearby pulsars at their early ages can form a bump-like feature in the spectrum due to radiative energy losses. In this paper, with a survey of nearby pulsars, we filter out four pulsars that may have notable contributions to ∼1.4 TeV cosmic ray electrons. Among them, PSR J0855−4644 has a spin-down luminosity more than 50 times higher than others and presumably dominates the electron fluxes from them. X-ray observations on the inner compact part (which may represent a tunnel for the transport of electrons from the pulsar) of PWN G267.0−01.0 are then used to constrain the spectral index of high-energy electrons injected by the pulsar. We show that high-energy electrons released by PSR J0855−4644 could indeed reproduce the 1.4 TeV spectral feature hinted by the DAMPE with reasonable parameters.

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36

Dong, J. N., Y. L. Zhang, Z. Y. Zhang, Y. F. Wei, L. B. Wu, C. Wang, Z. T. Shen et al. "Quality control of mass production of PMT modules for DAMPE". Journal of Instrumentation 12, n.º 05 (26 de mayo de 2017): T05004. http://dx.doi.org/10.1088/1748-0221/12/05/t05004.

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37

Yue, Chuan, Peng-Xiong Ma, Margherita Di Santo, Li-Bo Wu, Francesca Alemanno, Paolo Bernardini, Dimitrios Kyratzis, Guan-Wen Yuan, Qiang Yuan y Yun-Long Zhang. "Correction method for the readout saturation of the DAMPE calorimeter". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 984 (diciembre de 2020): 164645. http://dx.doi.org/10.1016/j.nima.2020.164645.

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38

Wei, Yifeng, Zhiyong Zhang, Yunlong Zhang, Chi Wang, Sicheng Wen, Jianing Dong, Zhiying Li et al. "Performance of the BGO Detector Element of the DAMPE Calorimeter". IEEE Transactions on Nuclear Science 63, n.º 2 (abril de 2016): 548–51. http://dx.doi.org/10.1109/tns.2016.2541690.

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39

Geng, Chao-Qiang, Da Huang y Lu Yin. "Multicomponent dark matter in the light of CALET and DAMPE". Nuclear Physics B 959 (octubre de 2020): 115153. http://dx.doi.org/10.1016/j.nuclphysb.2020.115153.

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40

Wang, Yuan-Peng, Si-Cheng Wen, Wei Jiang, Chuan Yue, Zhi-Yong Zhang, Yi-Feng Wei, YunLong Zhang, Jing-Jing Zang y Jian Wu. "Temperature effects on MIPs in the BGO calorimeters of DAMPE". Chinese Physics C 41, n.º 10 (28 de septiembre de 2017): 106001. http://dx.doi.org/10.1088/1674-1137/41/10/106001.

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41

Zhao, Yi, Xiao-Jun Bi, Su-Jie Lin y Peng-Fei Yin. "Nearby dark matter subhalo that accounts for the DAMPE excess". Chinese Physics C 43, n.º 8 (16 de julio de 2019): 085101. http://dx.doi.org/10.1088/1674-1137/43/8/085101.

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42

Ma, Peng-Xiong, Yong-Jie Zhang, Ya-Peng Zhang, Yao Li, Jing-Jing Zang, Xiang Li, Tie-Kuang Dong et al. "A method for aligning the plastic scintillator detector on DAMPE". Research in Astronomy and Astrophysics 19, n.º 6 (junio de 2019): 082. http://dx.doi.org/10.1088/1674-4527/19/6/82.

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43

Xu, Zhihui, Xiang Li, Mingyang Cui, Chuan Yue, Wei Jiang, Wenhao Li y Qiang Yuan. "An Unsupervised Machine Learning Method for Electron–Proton Discrimination of the DAMPE Experiment". Universe 8, n.º 11 (30 de octubre de 2022): 570. http://dx.doi.org/10.3390/universe8110570.

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Galactic cosmic rays are mostly made up of energetic nuclei, with less than 1% of electrons (and positrons). Precise measurement of the electron and positron component requires a very efficient method to reject the nuclei background, mainly protons. In this work, we develop an unsupervised machine learning method to identify electrons and positrons from cosmic ray protons for the Dark Matter Particle Explorer (DAMPE) experiment. Compared with the supervised learning method used in the DAMPE experiment, this unsupervised method relies solely on real data except for the background estimation process. As a result, it could effectively reduce the uncertainties from simulations. For three energy ranges of electrons and positrons, 80–128 GeV, 350–700 GeV, and 2–5 TeV, the residual background fractions in the electron sample are found to be about (0.45 ± 0.02)%, (0.52 ± 0.04)%, and (10.55 ± 1.80)%, and the background rejection power is about (6.21 ± 0.03) ×104, (9.03 ± 0.05) ×104, and (3.06 ± 0.32) ×104, respectively. This method gives a higher background rejection power in all energy ranges than the traditional morphological parameterization method and reaches comparable background rejection performance compared with supervised machine learning methods.

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44

Droz, D., A. Tykhonov, X. Wu, F. Alemanno, G. Ambrosi, E. Catanzani, M. D. Santo, D. Kyratzis y S. Zimmer. "A neural network classifier for electron identification on the DAMPE experiment". Journal of Instrumentation 16, n.º 07 (1 de julio de 2021): P07036. http://dx.doi.org/10.1088/1748-0221/16/07/p07036.

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45

Wei, Y. F., Z. Y. Zhang, Y. L. Zhang, S. C. Wen, C. Wang, Z. Y. Li, C. Q. Feng et al. "Temperature dependence calibration and correction of the DAMPE BGO electromagnetic calorimeter". Journal of Instrumentation 11, n.º 07 (5 de julio de 2016): T07003. http://dx.doi.org/10.1088/1748-0221/11/07/t07003.

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46

Ayazi, Seyed Yaser y Ahmad Mohamadnejad. "DAMPE excess from leptophilic vector dark matter: a model-independent approach". Journal of Physics G: Nuclear and Particle Physics 47, n.º 9 (22 de julio de 2020): 095003. http://dx.doi.org/10.1088/1361-6471/ab94cd.

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47

Wei, Yifeng, Yunlong Zhang, Zhiyong Zhang, Libo Wu, Sicheng Wen, Haoting Dai, Chenming Liu et al. "Performance of the DAMPE BGO calorimeter on the ion beam test". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 922 (abril de 2019): 177–84. http://dx.doi.org/10.1016/j.nima.2018.12.036.

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48

Zhang, Yongjie, Yuhong Yu, Zhiyu Sun, Yong Zhou, Fang Fang, Hongyun Zhao, Jie Kong et al. "Results of heavy ion beam tests of DAMPE plastic scintillator detector". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 953 (febrero de 2020): 163139. http://dx.doi.org/10.1016/j.nima.2019.163139.

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49

Zhang, Fei, Wen-Xi Peng, Ke Gong, Di Wu, Yi-Fan Dong, Rui Qiao, Rui-Rui Fan et al. "Design of the readout electronics for the DAMPE Silicon Tracker detector". Chinese Physics C 40, n.º 11 (noviembre de 2016): 116101. http://dx.doi.org/10.1088/1674-1137/40/11/116101.

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50

Zhang, De-Liang, Chang-Qing Feng, Jun-Bin Zhang, Qi Wang, Si-Yuan Ma, Zhong-Tao Shen, Di Jiang et al. "Onboard calibration circuit for the DAMPE BGO calorimeter front-end electronics". Chinese Physics C 40, n.º 5 (mayo de 2016): 056101. http://dx.doi.org/10.1088/1674-1137/40/5/056101.

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Artículos de revistas sobre el tema "DAMPE"

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