N. Produit, T. W. Bao, T. Batsch, T. Bernasconi, I. Britvich, F. Cadoux, I. Cernuda, J. Y. Chai, Y. W. Dong, N. Gauvin, W. Hajdas, M. Kole, M. N. Kong, R. Krame… 展开作者
N. Produit, T. W. Bao, T. Batsch, T. Bernasconi, I. Britvich, F. Cadoux, I. Cernuda, J. Y. Chai, Y. W. Dong, N. Gauvin, W. Hajdas, M. Kole, M. N. Kong, R. Kramert, L. Li, J. T. Liu, X. Liu, R. Marcinkowski, S. Orsi, M. Pohl, D. Rapin, D. Rybka, A. Rutczynska, H. L. Shi, P. Socha, J. C. Sun, L. M. Song, J. Szabelski, I. Traseira, H. L. Xiao, R. J. Wang, X. Wen, B. B. Wu, L. Zhang, L. Y. Zhang, S. N. Zhang, Y. J. Zhang, A. Zwolinska
The POLAR detector is a space based Gamma Ray Burst (GRB) polarimeter with a wide field of view, which covers almost half the sky. The instrument uses Compton scattering of gamma rays on a plastic scintillator hodoscope to measure the polarization of the incoming photons. The instrument has been successfully launched on board of the Chinese space laboratory Tiangong~2 on September 15, 2016. The construction of the instrument components is described in this article. Details are provided on problems encountered during the construction phase and their solutions. Initial performance of the instrument in orbit is as expected from ground tests and Monte Carlo simulation.
Using weighting algorithms to refine source direction determinations in all-sky gravitational wave burst searches with two-detector networks II: The case of elliptical polarization
Hard X-Ray Focal-Plane Compton Spectro-Polarimeter: Detector Development and Sensitivity Evaluation
Physical Research Laboratory（物理研究实验室）；INAF-IAPS（意大利国家天体物理研究所-空间天体物理研究所）；Kavli Institute of Particle Astrophysics and Cosmology, Stanford University（斯坦福大学卡弗里粒子天体物理学与宇宙学研究所）
Optimizing the light output of a plastic scintillator and SiPM based detector through optical characterization and simulation: A case study for POLAR-2
PolarLight: a CubeSat X-ray Polarimeter based on the Gas Pixel Detector
气体像元探测器（GPD）是为高灵敏度天文X射线偏振测量而设计和研制的，是近几年内即将打开的一扇新窗口。由于GPD的小质量，低功率和紧凑的几何形状，我们提出了一个立方体卫星任务偏振光（PolarLight）来演示和测试该技术直接在太空中。没有光学器件，只有一个准直器将视场限制在2.3度。充满0.8大气压的纯二甲醚（DME），并由100微米厚的铍窗密封，灵敏面积约为1.4 mm × 1.4 mm，PolarLight允许我们观察天空中最亮的X射线源，计数率为，例如，~0.2计数/秒来自蟹状星云。PolarLight大小为1U，安装在6 U CubeSat上，于2018年10月29日发射到低地球太阳同步轨道，目前正在测试中。计划在2019年推出更多改进设计的产品。这些测试将有助于提高未来任务的技术准备程度，如增强型X射线定时和偏振测量（eXTP），更好地了解轨道背景，并可能有助于通过观测最亮物体来限制物理学。
Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
College of Physics, Chongqing University（重庆大学物理学院）；Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University（重庆大学物理系及强耦合物理重庆市重点实验室）
Seasonal Variation of Polar Ice: Implications for Ultrahigh Energy Neutrino Detectors
Interuniversity Institute for High Energies, Université Libre de Bruxelles（高能大学间研究所，布鲁塞尔自由大学）；Dept. of Physics and Astronomy, University of Kansas（堪萨斯大学物理与天文学系）
Structured generalized sliced Wasserstein distance for keV X-ray polarization analysis with Gas Pixel Detector
Central China Normal University（华中师范大学）；Hubei Provincial Engineering Research Center of Silicon Pixel Chip & Detection Technology（湖北省硅像素芯片与探测技术工程研究中心）；Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University（广西大学物理科学与技术学院相对论天体物理学重点实验室）
Development of a one-dimensional position sensitive detector for Compton X-ray polarimeters
Physical Research Laboratory（物理研究实验室）；INAF − - Istituto di Astrofisica e Planetologia Spaziali di Roma（罗马天体物理学和行星学研究所）；Kavli Institute of Particle Astrophysics and Cosmology, Stanford University（斯坦福大学卡弗里粒子天体物理学与宇宙学研究所）
