Lin,Chih-Hsun / Senior Research Scientist

Research Interest

• High energy experiments, Radiation hard electronics and testing, detectors for radiotherapy

獎項及殊榮

Experience

• 10/1999 – 07/2003Postdoctoral Associate at National Central University
• 08/2003 – 08/2005Assistant Research Scientist of National Science Council
• 09/2005 – 07/2009Associate Researcher at National Space Organization

Publication

Journal Papers

• [1]     Yi-Chun Lin, C.Y. Pan, K.J. Chiang, M.C. Yuan, C.H. Chu, Y.W. Tsai, P.K. Teng, C.H. Lin, T.C. Chao, C.C. Lee, C.J. Tung, A.E. Chen, accepted, “Monte Carlo simulations for angular and spatial distributions in therapeutic-energy proton beams”, RADIATION PHYSICS AND CHEMISTRY, 140, 217-224. (SCIE) (IF: 1.315; SCIE ranking: 24.2%,72.2%,75.3%)
  
  
• [2]     Chien-Ying Yang, Yi-Chi Chang, Hung-Hsiang Liang, Che-Yen Chu, Jr-Yue Hsiang, Jeng-Lun Chiu, Chih-Hsun Lin,Philippe Laurent,Jerome Rodriguez, Hsiang-Kuang Chang, 2020, “Feasibility of Observing Gamma-Ray Polarization from Cygnus X-1 Using a CubeSat”, ASTRONOMICAL JOURNAL, 160:54. (SCIE) (IF: 4.15; SCIE ranking: 25.8%)
  
  
• [3]     AMS Collaboration, 2020, “Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer”, PHYSICAL REVIEW LETTERS, 124, 211102. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [4]     AMS Collaboration, 2019, “Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer”, PHYSICAL REVIEW LETTERS, 123,181102. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [5]     AMS Collaboration, 2019, “Towards Understanding the Origin of Cosmic-Ray Electrons”, PHYSICAL REVIEW LETTERS, 122.101101. (SCIE) (IF: 8.839; SCIE ranking: 9.5%)
  
  
• [6]     AMS Collaboration, 2019, “Towards Understanding the Origin of Cosmic-Ray Positrons”, PHYSICAL REVIEW LETTERS, 122.041102. (SCIE) (IF: 8.839; SCIE ranking: 9.5%)
  
  
• [7]     AMS Collaboration, 2018, “Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051102. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [8]     AMS Collaboration, 2018, “Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051101. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [9]     AMS Collaboration, 2018, “Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051103. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [10]     AMS Collaboration, 2018, “Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 120,021101. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [11]     AMS Collaboration, 2017, “Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 119, 251101. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [12]     AW Lowell et al., 2017, “Maximum Likelihood Compton Polarimetry with the Compton Spectrometer and Imager”, ASTROPHYSICAL JOURNAL, 848(2), 120. (SCIE) (IF: 5.533; SCIE ranking: 11.1%)
  
  
• [13]     AW Lowell et al., 2017, “Polarimetric Analysis of the Long Duration Gamma-Ray Burst GRB 160530A With the Balloon Borne Compton Spectrometer and Imager”, ASTROPHYSICAL JOURNAL, 848(2), 119. (SCIE) (IF: 5.533; SCIE ranking: 11.1%)
  
  
• [14]     AMS Collaboration, 2016, “Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 117, 231102. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [15]     AMS Collaboration, 2016, “Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station ”, PHYSICAL REVIEW LETTERS, 117,091103. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [16]     AMS Collaboration, 2015, “Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV”, PHYSICAL REVIEW LETTERS, 115, 211101. (SCIE) (IF: 8.462; SCIE ranking: 7.6%)
  
  
• [17]     J.-L. Chiu et al. COSI collaboration, 2015, “The upcoming balloon campaign of the Compton Spectrometer and Imager (COSI)”, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 784, 359-363. (SCIE) (IF: 1.336; SCIE ranking: 30.3%,67.2%,70%,82.8%)
  
  
• [18]     M. Aguilar et al. AMS Collaboration, 2015, “ Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station ”, PHYSICAL REVIEW LETTERS, 114, 171103. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [19]     AMS collaboration, 2014, “Precision Measurement of the (e(+) + e(-)) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 221102. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [20]     M. Aguilar et al. AMS Collaboration, 2014, “Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 121102. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [21]     L. Accardo et al. AMS Collaboration, 2014, “High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–500 GeV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 121101. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [22]     ALEPH Collaboration ; DELPHI Collaboration ; L3 Collaboration ; OPAL Collaboration ; LEP Electroweak Working Grp, 2013, “Electroweak measurements in electron positron collisions at W-boson-pair energies at LEP”, PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 532(4), 119-244. (SCIE) (IF: 20.099; SCIE ranking: 3.8%)
  
  
• [23]     ALEPH and DELPHI and L3 and OPAL and LEP Electroweak Working Group Collaborations, 2013, “Search for Charged Higgs bosons: Combined Results Using LEP Data ”, EUROPEAN PHYSICAL JOURNAL C, 73:2463. (SCIE) (IF: 5.172; SCIE ranking: 17.2%)
  
  
• [24]     M. Aguilar et al. AMS Collaboration , 2013, “First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV”, PHYSICAL REVIEW LETTERS, 110, 141102. (SCIE) (IF: 8.839; SCIE ranking: 7.7%)
  
  
• [25]     L3 collaboration, 2011, “Generalized event shape and energy flow studies in e+e− annihilation at √s=91.2−208.0 GeV”, JOURNAL OF HIGH ENERGY PHYSICS, 143. (SCIE) (IF: 5.541; SCIE ranking: 13.8%)
  
  
• [26]     M. S. Bandstra, E. C. Bellm, S. E. Boggs, D. Perez-Becker, A. Zoglauer, H.-K. Chang, J.-L. Chiu, J.-S. Liang, Y.-H. Chang, Z.-K. Liu, W.-C. Hung, M.-H. A. Huang, S. J. Chiang, R.-S. Run, C.-H. Lin, M. Amman, P. N. Luke,P. Jean, P. von Ballmoos, and C. B. Wunderer, 2011, “DETECTION AND IMAGING OF THE CRAB NEBULA WITH THE NUCLEAR COMPTON TELESCOPE”, ASTROPHYSICAL JOURNAL, 738(1), 8. (SCIE) (IF: 5.551; SCIE ranking: 16.7%)
  
  
• [27]     M. Aguilar et al., 2011, “ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01”, ASTROPHYSICAL JOURNAL, 736(2),105. (SCIE) (IF: 5.551; SCIE ranking: 16.7%)
  
  
• [28]     The L3 Collaboration, 2011, “Test of the τ-model of Bose–Einstein correlations and reconstruction of the source function in hadronic Z-boson decay at LEP”, EUROPEAN PHYSICAL JOURNAL C, 71(5), 1648. (SCIE) (IF: 5.172; SCIE ranking: 17.2%)
  
  
• [29]     M. Aguilar et al., 2010, “RELATIVE COMPOSITION AND ENERGY SPECTRA OF LIGHT NUCLEI IN COSMIC RAYS:”, ASTROPHYSICAL JOURNAL, 724,329-340. (SCIE) (IF: 5.551; SCIE ranking: 16.7%)
  
  
• [30]     Wei-Che Hung; Yuan-Hann Chang; "Chih-Hsun Lin"; Boggs, S.E.; Hsiang-Kuang Chang; Bandstra, M.S.; Bellm, E.C.; Jeng-Lun Chiu; Jau-Shian Liang; Zong-Kai Liu; Perez-Becker, D.; Wunderer, C.B.; Zoglauer, A.; Ming-Huey Huang; Amman, M.; Luke, P.N.;, 2009, “The Data Readout System of the Nuclear Compton Telescope (NCT)”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 56(04), 2303-2308. (SCIE) (IF: 1.44; SCIE ranking: 18.2%,61.9%)
  
  
• [31]     Zong-Kai Liu, Yuan-Hann Chang, Boggs S.E., Bandstra M.S., Bellm E.C., Bowen J.D., Perez-Becker D., Wunderer C.B., Zoglauer A., Amman M., Luke P.N., Hsiang-Kuang Chang, Jeng-Lun Chiu, Jau-Shian Liang, "Chih-Hsun Lin", Wei-Che Hung, 2009, “Characterizing and Correcting the Cross-Talk Effect on Depth Measurement in the NCT Detectors”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, Volume 56, Issue 3, Part 2, 1210-1214. (SCIE) (IF: 1.44; SCIE ranking: 18.2%,61.9%)
  
  
• [32]     Bellm, E.C., Boggs, S.E., Bandstra, M.S., Bowen, J.D., Perez-Becker, D., Wunderer, C.B., Zoglauer, A., Amman, M., Luke, P.N., Hsiang-Kuang Chang, Jeng-Lun Chiu, Jau-Shian Liang, Yuan-Hann Chang, Zong-Kai Liu, Wei-Che Hung, "Chih-Hsun Lin", Huang, M.A.,Jean, P., 2009, “Overview of the Nuclear Compton Telescope”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, Volume 56, Issue 3, Part 2, 1250-1256. (SCIE) (IF: 1.44; SCIE ranking: 18.2%,61.9%)
  
  

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