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The flux modulation of INTEGRAL

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Science China(Physics,Mechanics & Astronomy) 2010年第S1期53卷 110-113页

作者： CHEN YuPeng,ZHANG Shu,WANG JianMin,LI TiPei & qu jinlu Laboratory for Particle Astrophysics,Institute of High Energy Physics,Beijing 100049,China Laboratory for Particle Astrophysics Institute of High Energy Physics Beijing China

We have analyzed International Gamma-Ray Astrophysics Laboratory(INTEGRAL) data corresponding to observations of the high mass X-ray binary(HMXB) V0332+53 during its huge outburst which occurred in 2004-2005,and found that there is a quasi periodic signal with ultra low frequency of roughly 4-5×10-5 Hz in the *** feature is revealed through a series of consistent analyses of imagings and fittings of the energy spectrum for each science window(SCW),and shows up in the corresponding light *** analysis of the power spectrum also provides a hint of a power peak located around 4×10-5 Hz,after subtracting off the linear trend of the light curve,and shows the consistency with the previous analyses.A similar feature shows up in our analysis of the light curve of Crab in hexagonal dithering ***,an instrumental effect on the flux modulation might exist in the INTEGRAL data product of different levels:imaging,spectral fitting and light curve analysis,at least for the observational mode of hexagonal *** an effect is,to our knowledge,not yet available in the current literature.

关键词： X-ray source individual V0332+53

A Possible 250s X-Ray quasi-periodicity in the Fast Blue Optical Transient AT2018cow

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Research in Astronomy and Astrophysics 2022年第12期22卷 299-310页

作者： Wenjie Zhang Xinwen Shu Jin-Hong Chen Luming Sun Rong-Feng Shen Lian Tao Chun Chen Ning Jiang Liming Dou Ying Qin Xue-Guang Zhang Liang Zhang jinlu qu Tinggui Wang Department of Physics Anhui Normal UniversityWuhu 241002China School of Physics and Astronomy Sun Yat-Sen UniversityZhuhai 519082China Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of ScienceBeijing 100049China CAS Key Laboratory for Researches in Galaxies and Cosmology Department of AstronomyUniversity of Science and Technology of ChinaHefei 230026China Department of Astronomy Guangzhou UniversityGuangzhou 510006China School of Physics and Technology Nanjing Normal UniversityNanjing 210023China

The fast blue optical transients(FBOTs)are a new population of extragalactic transients of unclear physical origin.A variety of mechanisms has been proposed including failed supernova explosion,shock interaction with a dense medium,young magnetar,accretion onto a compact object and stellar tidal disruption event,but none is *** we report the discovery of a possible X-ray quasi-periodicity signal with a period of~250 s(at a significance level of 99.76%)in the brightest FBOT AT2018cow through the analysis of XMM-Newton/PN *** signal is independently detected at the same frequency in the average power density spectrum from data taken from the Swift telescope,with observations covering from 6 to 37 days after the optical discovery,though the significance level is lower(94.26%).This suggests that the quasi-periodic oscillation(QPO)frequency may be stable over at least 1.1×10^(4)*** the~250 s QPO to be a scaled-down analog of that typically seen in stellar mass black holes,a black hole mass of~103–10^(5)solar masses could be *** overall X-ray luminosity evolution could be modeled with a stellar tidal disruption by a black hole of~10^(4)solar masses,providing a viable mechanism to produce *** findings suggest that other bright FBOTs may also harbor intermediate-mass black holes.

关键词： black hole physics X-rays:individual(AT2018cow) X-rays:bursts

Simulation of the in-flight calibration of the collimator alignment and PSF for HXMT

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Science China(Physics,Mechanics & Astronomy) 2010年第S1期53卷 47-50页

作者： XIONG ShaoLin,LI XinQiao,qu jinlu & LU FangJun Key Laboratory for Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China Key Laboratory for Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences (CAS) Beijing China

The Hard X-ray Modulation Telescope(HXMT) is an X-ray astronomical satellite in 1-250 keV,consisting of three collimated *** present the in-flight calibration approach of the collimator alignment and Point Spread Function(PSF) for HXMT,using both the direct fitting method and the imaging *** to observational simulations of the Crab Nebula,we find that these two methods produce almost the same calibration accuracy of the alignment,and with a one-day scanning observation,the alignment can be calibrated to better than 0.45' and 0.1' along the wide and narrow directions of the Field of View(FOV) for a detector module,which corresponds to a localization accuracy of better than 0.1' and meets the scientific requirement.

关键词： HXMT alignment PSF calibration

The rms-flux relation of Cyg X-2 in the horizontal branch

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Science China(Physics,Mechanics & Astronomy) 2010年第S1期53卷 86-90页

作者： LI ZhiBing,LEI YaJuan,qu jinlu,ZHANG Shu & SONG LiMing Key Laboratory for Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China Key Laboratory for Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences (CAS) Beijing China

We have investigated the relation between the root mean square(rms) variability and the X-ray flux(rms-flux relation) of the Z source Cyg X-2,and as well the energy dependence based on the Rossi X-ray Timing Explorer(RXTE) *** currently focus on the horizontal branch(HB),due to the negative correlation in flux of the soft and the hard *** rms-flux correlation has energy dependence as follows:positive at hard X-rays(above 10 keV) but negative at soft X-rays(below 10 keV).This provides a feature different from the previous one,and may be suggestive of different origins of X-rays below and above 10 ***,the overall spectrum can be well fitted with a model consisting of a blackbody and Comptonization components,but the fitting results do not reveal any features around 10 keV that could account for such a change in the rms-flux relation.

关键词： accretion accretion disk—binaries:close-stars:individual(Cygnus X-2)-X-rays:binaries

The Medium Energy X-ray telescope (ME) onboard the Insight-HXMT astronomy satellite

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Science China(Physics,Mechanics & Astronomy) 2020年第4期63卷 35-48页

作者： XueLei Cao WeiChun Jiang Bin Meng WanChang Zhang Tao Luo Sheng Yang ChunLei Zhang YuDong Gu Liang Sun XiaoJing Liu JiaWei Yang Xian Li Ying Tan ShaoZhen Liu YuanYuan Du FangJun Lu YuPeng Xu Ju Guan ShuangNan Zhang HuanYu Wang TiPei Li ChengMo Zhang XiangYang Wen jinlu qu LiMing Song XiaoBo Li MingYu Ge YuPeng Zhou ShaoLin Xiong Shu Zhang YongJie Zhang ZeHao Cheng Fei Zhang MaoShun Li XiaoHua Liang Min Gao EnBo Yang XiaoHang Liu HongWei Liu YiJung Yang Fan Zhang Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Beijing Key Laboratory of Space Thermal Control Technology Beijing Institute of Spacecraft System EngineeringBeijing 100094China Department of Modern Physics School of Physical SciencesUniversity of Science and Technology of ChinaHefei 230022China School of Physical Sciences Guizhou UniversityGuivang 550025China School of Opto-Electronic Information Science and Technology Yantai UniversityYantai 264005China University of Chinese Academy of Sciences Beijing 100049China

The Medium Energy X-ray telescope(ME) is one of the three main telescopes on board the Insight hard X-ray modulation telescope(Insight-HXMT) astronomy satellite. ME contains 1728 pixels of Si-PIN detectors sensitive in 5-30 ke V with a total geometrical area of 952 cm^2. The application specific integrated circuit(ASIC) chip, VA32TA6, is used to achieve low power consumption and low readout noise. The collimators define three kinds of field of views(FOVs) for the telescope, 1°×4°, 4°×4°,and blocked ones. Combination of such FOVs can be used to estimate the in-orbit X-ray and particle background *** energy resolution of ME is ~3 ke V at 17.8 ke V(FWHM) and the time resolution is 255 μs. In this paper, we introduce the design and performance of ME.

关键词： Si-PIN ASIC medium energy X-ray

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HXMT卫星长期任务规划算法

空间科学学报 2017年第6期37卷 766-772页

作者：黄跃屈进禄贾淑梅马想宋黎明陈黎张文昭中国科学院高能物理研究所粒子天体物理重点实验室北京100049 北京师范大学天文学系北京100875

硬X射线调制望远镜(HXMT)卫星是中国首颗空间X射线天文卫星.为充分利用卫星资源,使科学产出最大化,需要进行长期任务规划.长期任务规划是一个复杂的多目标优化问题.通过分析HXMT观测特点和约束条件,建立了HXMT长期任务规划问题模型,并... 详细信息

硬X射线调制望远镜(HXMT)卫星是中国首颗空间X射线天文卫星.为充分利用卫星资源,使科学产出最大化,需要进行长期任务规划.长期任务规划是一个复杂的多目标优化问题.通过分析HXMT观测特点和约束条件,建立了HXMT长期任务规划问题模型,并采用贪婪算法加遗传算法对模型进行求解.实例分析结果表明该方法能够有效解决HXMT长期任务规划问题.

关键词：硬X射线调制望远镜长期任务规划贪婪算法遗传算法

Boosting bidirectional sulfur conversion enabled by introducing boron-doped atoms and phosphorus vacancies in Ni2P for lithium-sulfur batteries

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Journal of Energy Chemistry 2025年第1期100卷 760-769页

作者： Lin Peng Yu Bai Hang Li Meixiu qu Zhenhua Wang Kening Sun Advanced Research Institute of Multidisciplinary Science Beijing Institute of Technology Beijing Key Laboratory of Chemical Power Source and Green Catalysis School of Chemistry and Chemical Engineering Beijing Institute of Technology

Lithium-sulfur （Li-S） batteries have gained great attention due to the high theoretical energy density and low cost,yet their further commercialization has been obstructed by the notorious shuttle effect and sluggish redox ***,we supply a strategy to optimize the electron structure of Ni2P by concurrently introducing B-doped atoms and P vacancies in Ni2P （Vp-B-Ni2P）,thereby enhancing the bidirectional sulfur *** study indicates that the simultaneous introduction of B-doped atoms and P vacancies in Ni2P causes the redistribution of electron around Ni atoms,bringing about the upward shift of d-band center of Ni atoms and effective d-p orbital hybridization between Ni atoms and sulfur species,thus strengthening the chemical anchoring for lithium polysulfides （LiPSs） as well as expediting the bidirectional conversion kinetics of sulfur ***,theoretical calculations reveal that the incorporation of B-doped atoms and P vacancies in Ni2P selectively promotes Li2S dissolution and nucleation ***,the Li-S batteries with Vp-B-Ni2P-separators present outstanding rate ability of 777 m A h g-1at 5 C and high areal capacity of 8.03 mA h cm-2under E/S of 5μL mg-1and sulfur loading of 7.20 mg *** work elucidates that introducing heteroatom and vacancy in metal phosphide collaboratively regulates the electron structure to accelerate bidirectional sulfur conversion.

关键词： Lithium sulfur batteries

硬X射线调制望远镜卫星科学观测应用初步评价

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航天器工程 2018年第5期27卷 168-174页

作者：贾淑梅黄跃马想屈进禄宋黎明张澍郑世界葛明玉中国科学院高能物理研究所北京100049

硬X射线调制望远镜(HXMT)卫星已顺利在轨运行1年多,完成了核心科学目标观测。文章概述了HXMT卫星的观测情况,如顺利完成核心观测源和银道面扫描的观测;重点介绍在银道面扫描、黑洞和中子星双星时变与能谱分析、伽马射线暴探测及引力波... 详细信息

硬X射线调制望远镜(HXMT)卫星已顺利在轨运行1年多,完成了核心科学目标观测。文章概述了HXMT卫星的观测情况,如顺利完成核心观测源和银道面扫描的观测;重点介绍在银道面扫描、黑洞和中子星双星时变与能谱分析、伽马射线暴探测及引力波电磁对应体研究、脉冲星观测及脉冲星导航试验等方面获得的初步成果。HXMT卫星与国外空间X射线望远镜卫星及国内外地面望远镜开展的联合观测,促进了HXMT卫星的标定工作。HXMT卫星在黑洞与中子星研究、伽马射线暴探测及银河系内新源与暴发源监测方面会发挥重要作用。

关键词：硬X射线调制望远镜卫星 X射线双星脉冲星伽马射线暴引力波

硬X射线调制望远镜卫星地面科学应用部分设计与应用

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航天器工程 2018年第5期27卷 162-167页

作者：郑世界贾淑梅马想聂建胤李小波李兵屈进禄宋黎明中国科学院高能物理研究所北京100049

根据硬X射线调制望远镜(HXMT)卫星开展科学观测的需求,提出了地面应用系统科学应用部分的设计方案,包括总体架构、外部接口、功能组成及主要工作流程等。在轨测试阶段的测试结果分析与验证表明,科学应用部分工作正常,实现了有效载荷的... 详细信息

根据硬X射线调制望远镜(HXMT)卫星开展科学观测的需求,提出了地面应用系统科学应用部分的设计方案,包括总体架构、外部接口、功能组成及主要工作流程等。在轨测试阶段的测试结果分析与验证表明,科学应用部分工作正常,实现了有效载荷的在轨监测与参数调整、科学观测计划制定、数据产品生成与数据分析等功能,能为HXMT卫星的在轨正常运行及开展科学研究提供保障。

关键词：硬X射线调制望远镜卫星科学应用部分在轨监测数据分析