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Yu Lu1,2,3,Yun-Zhao Wu1,4,Cui Li1,Jin-Song Ma5,6,Wen-Wen Qi7,Wei Tan7,Xiao-Man Li7,Zhi-Cheng Shi7,Hong-Yan He7,Shu-Wu Dai8,Guo Li8,Feng-Jing Liu8,Jing-Qiao Wang9,Xiao-Yan Wang9,Qi Wang10,Ling-Jie Meng10(Key Laboratory of Planetary Sciences,Purple Mountain Observatory,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Science and Technology of China;CAS Center for Excellence in Comparative Planetology;Space Science Institute,Macau University of Science and Technology;School of Geography and Ocean Science,Nanjing University;Jiangsu Center for Collaborative Innovation in Geographical Information Resource Development and Application;Beijing Institute of Space Mechanics and Electricity;Beijing Institute of Spacecraft System Engineering;China Centre for Resources Satellite Data and Application;Earth Observation System and Data Center,China National Space Administration).Seamless maps of major elements of the Moon:Results from high-resolution geostationary satellite[J].天文和天体物理学研究(英文版),2021,第2期
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Tian-Yi Chen1,2,Jian-Rong Shi1,2,Timothy C.Beers3,Hong-Liang Yan1,2,Qi Gao1,2,Chun-Qian Li1,2,Hai-Ning Li1,Gang Zhao1,2(CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences;Department of Physics and JINA Center for the Evolution of the Elements,University of Notre Dame).Searching for r-process-enhanced stars in the LAMOST survey I:the method[J].天文和天体物理学研究(英文版),2021,第2期
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Guo Yunlang,Liu Dongdong,Wu Chengyuan,Wang Bo.He-shell flashes on the surface of oxygen-neon white dwarfs[J].天文和天体物理学研究,2021,第2期
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Miao Li1,Yu-Kun Huang2,Sheng-Ping Gong1(School of Aerospace Engineering,Tsinghua University;Department of Physics and Astronomy,University of British Columbia).A semi-analytic model for the study of 1/1 resonant dynamics of the planar elliptic restricted co-orbital problem[J].天文和天体物理学研究(英文版),2021,第2期
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Xiao Zhou1,2,3,Sheng-Bang Qian1,2,3,4(Yunnan Observatories,Chinese Academy of Sciences (CAS);Key Laboratory of the Structure and Evolution of Celestial Objects,Chinese Academy of Sciences;Center for Astronomical Mega-Science,Chinese Academy of Sciences;University of the Chinese Academy of Sciences).Orbital period correction and light curve modeling of the W-subtype shallow contact binary OW Leo[J].天文和天体物理学研究(英文版),2021,第2期
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Chun-Yan Lu,Jing-Wen Yan,Lu Wen,Jun Fang(Department of Astronomy,Key Laboratory of Astroparticle Physics of Yunnan Province,Yunnan University).Numerically investigating the peculiar periphery of a supernova remnant in the medium with a density gradient:the case of RCW 103[J].天文和天体物理学研究(英文版),2021,第2期
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孙立早1,2,黄乘利3,2,于涌3,2,齐朝祥3,2,唐正宏1,2,赵铭1,杨德华4,吴彤5(Shanghai Astronomical Observatory,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences;CAS Key Laboratory of Planetary Sciences,Shanghai Astronomical Observatory,Chinese Academy of Sciences;College of Automation Engineering,Nanjing University of Aeronautics and Astronautics;Key Laboratory of Space Photoelectric Detection and Sensing of Ministry of Industry and Information Technology,College of Astronautics,Nanjing University of Aeronautics and Astronautics).A new telescope with three fields of view to measure the orientation parameters of the Moon and terrestrial planets[J].天文和天体物理学研究(英文版),2021,第2期
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Lin-Cheng Li1,2,3,Bo Qin1,Jie Wang1,2,Jing Wang4,You-Gang Wang1(National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences;International Centre for Radio Astronomy Research (ICRAR),The University of Western Australia;Department of Astronomy,Peking University).The conformity of H I galaxies in ALFALFA-SDSS sample[J].天文和天体物理学研究(英文版),2021,第2期
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Lin-Cheng Li1,2,3,4,Lister Staveley-Smith3,4,5,Jonghwan Rhee3,4,5(National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences;International Centre for Radio Astronomy Research (ICRAR),The University of Western Australia,35 Stirling Hwy;ARC Centre of Excellence for All-sky Astrophysics (CAASTRO);ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)).An HI intensity mapping survey with a Phased Array Feed[J].天文和天体物理学研究(英文版),2021,第2期
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Zheng-Xiong Sun1,Jin-Qing Wang1,2,3,Lin-Feng Yu1,Wei Gou1,Guang-Li Wang1,4(Shanghai Astronomical Observatory,Chinese Academy of Sciences;Key Laboratory of Radio Astronomy,Chinese Academy of Sciences;Shanghai Key Laboratory of Space Navigation and Positioning Techniques;University of Chinese Academy of Sciences).Research on the panel adjustment method of an active main reflector for a large radio telescope[J].天文和天体物理学研究(英文版),2021,第2期
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Rui Liu(CAS Key Laboratory of Geospace Environment;CAS Center for Excellence in Comparative Planetology;Mengcheng National Geophysical Observatory).Erratum:“Magnetic flux ropes in the solar corona:structure and evolution toward eruption”(2020,RAA,20,165)[J].Research in Astronomy and Astrophysics,2021,第2期
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Nan-Nan Yue1,2,Yang Gao3,Di Li1,2,4,Liu-Bin Pan3(National Astronomical Observatories,Chinese Academy of Sciences;University of Chinese Academy of Sciences;School of Physics and Astronomy,Sun Yat-Sen University;NAOC-UKZN Computational Astrophysics Centre,University of Kwa Zulu-Natal).Collapsing index:a new method to identify star-forming cores based on ALMA images[J].天文和天体物理学研究(英文版),2021,第2期
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Hui Li,Bo Chen,Li Feng,Ying Li,Yu Huang,Jing-Wei Li,Lei Lu,Jian-Chao Xue,Bei-Li Ying,Jie Zhao,Yu-Tong Yang,Wei-Qun Gan,Cheng Fang,Ke-Fei Song,Hong Wang,Quan-Feng Guo,Ling-Ping He,Bo Zhu,Cheng Zhu,Lei Deng,Hai-Chao Bao,Cai-Xia Cao,Zhong-Guang Yang(China;China Received 2019 June 28;accepted2019 July 25).Erratum:“The Lyman-alpha Solar Telescope(LST)for the ASO-S mission—I.Scientific objectives and overview”(2019,RAA,19,158)[J].Research in Astronomy and Astrophysics,2021,第2期
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Biswajit Das,Biswajit Pandey(Department of Physics Visva-Bharati University Department of Physics Visva-Bharati University).Can we constrain the evolution of HI bias using configuration entropy?[J].Research in Astronomy and Astrophysics,2021,第2期
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Abhijit Bandyopadhyay,Anirban Chatterjee(Department of Physics,Ramakrishna Mission Vivekananda Educational and Research Institute).Time-dependent diffusive interactions between dark matter and dark energy in the context of k-essence cosmology[J].天文和天体物理学研究(英文版),2021,第1期
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Yong-Gang Zheng1,2,3,4,Chu-Yuan Yang1,4,Shi-Ju Kang5,Jin-Ming Bai1,4(Yunnan Observatories,Chinese Academy of Sciences;Department of Physics,Yunnan Normal University;Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment-Shandong University;Key Laboratory for the Structure and Evolution of Celestial Objects,Chinese Academy of Sciences;Department of Physics and Electronics Science,Liupanshui Normal University).An explanation for 13 consecutive day activities of Mrk 421[J].天文和天体物理学研究(英文版),2021,第1期
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Qiao Wang(Key Laboratory for Computational Astrophysics,National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences).A hybrid Fast Multipole Method for cosmological N-body simulations[J].天文和天体物理学研究(英文版),2021,第1期
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Bo Han1,Li-Na Qiao1,Jing-Lin Chen1,Xian-Da Zhang2,Yan-Xia Zhang3,Yong-Heng Zhao3(School of Computer Science,Wuhan University;Institute of Electronics,Chinese Academy of Sciences;CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences).GeneticKNN:a weighted KNN approach supported by genetic algorithm for photometric redshift estimation of quasars[J].天文和天体物理学研究(英文版),2021,第1期
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Wei Duan1,2,3,Qian Song1,2,3,Ming-Zhi Wei1,Zhao-Wang Zhao1,3,Wei Wang1,3,Yu-Heng Zhang1,3,Zhi-Wei Feng1,2,3(National Astronomical Observatories,Chinese Academy of Sciences;University of Chinese Academy of Sciences;CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories).Research on the readout noise suppression method for digital correlated double sampling[J].天文和天体物理学研究(英文版),2021,第1期
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Dugasa Belay Zeleke,Solomon Belay Tessema ,Seblu Humne Negu(Received2020 February 4;accepted2020 July 2).Effects of dynamo magnetic f elds on observational properties of accreting millisecond X-ray pulsars[J].Research in Astronomy and Astrophysics,2021,第1期
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Qi-Jie Wang,Jia-Chen Li , Liang-Qi Guo(School of Geosciences and Info-Physics,Central South University).Solar cycle prediction using a long short-term memory deep learning model[J].天文和天体物理学研究(英文版),2021,第1期
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Ke-Rui Zhu1,Shi-Ju Kang2,Yong-Gang Zheng1(Department of Physics,Yunnan Normal University;School of Physics and Electrical Engineering,Liupanshui Normal University).Searching for AGN and pulsar candidates in 4FGL unassociated sources using machine learning[J].天文和天体物理学研究(英文版),2021,第1期
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Deng-Ke Zhou1,2,Shi-Jie Zheng1,Li-Ming Song1,2,Yong Chen1,Cheng-Kui Li1,Xiao-Bo Li1,Tian-Xiang Chen1,Wei-Wei Cui1,Wei Chen1,2,Da-Wei Han1,Wei Hu1,Jia Huo1,Rui-Can Ma1,2,Mao-Shun Li1,Tian-Ming Li1,2,Wei Li1,He-Xin Liu1,2,Bo Lu1,Fang-Jun Lu1,Jin-Lu Qu1,2,You-Li Tuo1,2,Juan Wang1,Yu-Sa Wang1,Bai-Yang Wu1,2,Guang-Cheng Xiao1,2,Yu-Peng Xu1,Yan-Ji Yang1,Shu Zhang1,Zi-Liang Zhang1,Xiao-Fan Zhao1,2,Yu-Xuan Zhu1,3(China;China Received 2020 April 28;accepted2020 July 2).The inf uence of the Insight-HXMT/LE time response on timing analysis[J].Research in Astronomy and Astrophysics,2021,第1期
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Yu Wang1,2,3,Hai-Yan Zhang2,3,Hao Hu2,Shi-Jie Huang2,Wei-Wei Zhu2,3,Guo-Ping Zhi4,Tao Zhang4,Zhan-Chun Fan4,Li Yang2,3(University of Chinese Academy of Sciences;National Astronomical Observatories,Chinese Academy of Sciences;CAS Key Laboratory of FAST,National Astronomical Observatories,Chinese Academy of Sciences;Beijing Institute of Spacecraft System Engineering).Satellite RFI mitigation on FAST[J].天文和天体物理学研究(英文版),2021,第1期
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Ying-Hua Yue1,Sheng-Li Qin1,Tie Liu2,Meng-Yao Tang1,Yuefang Wu3,Ke Wang4,Chao Zhang1(Department of Astronomy,Yunnan University,and Key Laboratory of Astroparticle Physics of Yunnan Province;Shanghai Astronomical Observatory,Chinese Academy of Sciences;Department of Astronomy,Peking University;Kavli Institute for Astronomy and Astrophysics,Peking University).Infall in massive clumps harboring bright infrared sources[J].天文和天体物理学研究(英文版),2021,第1期
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苏艳蕊1,2,王强3,严发宝1,2,4,黄永梅3(School of Mechanical,Electrical & Information Engineering,Shandong University;Laboratory for Electrom Agnetic Detection,Institute of Space Sciences,Shandong University;Institute of Optics and Electronics,Chinese Academy of Sciences;CAS Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences).Friction compensation for an m-Level telescope based on high-precision LuGre parameters identification[J].天文和天体物理学研究(英文版),2021,第1期
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Xin-Wei Zhang1,2,Yang Zhang2,Jia-Ben Lin2,Jun-Feng Hou1,2,Yuan-Yong Deng1,2(Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Science,University of Chinese Academy of Sciences).Research on the principle of space high-precision temperature control system of liquid crystals based Stokes polarimeter[J].天文和天体物理学研究(英文版),2021,第1期
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Dao-Ye Yang1,2,3,Li-Fang Li1,2,4,5,Quan-Wang Han6(Yunnan Observatories,Chinese Academy of Sciences;Key Laboratory for the Structure and Evolution of Celestial Objects,Chinese Academy of Sciences;University of Chinese Academy of Sciences;Center for Astronomical Mega-Science,Chinese Academy of Sciences;Key Lab of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;School of Physics and Electronics,Qiannan Normal University for Nationalities).Absolute physical parameters of three poorly studied detached eclipsing binaries[J].天文和天体物理学研究(英文版),2021,第1期
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Shuo-Ran Yu, Xiao-Ping Zhang(State Key Laboratory of Lunar and Planetary Sciences,Macau University of Science and Technology).Effects of initial velocity on the sinking of ilmenite-bearing cumulates in the early lunar mantle:Insight from the theory of Rayleigh-Taylor instability[J].天文和天体物理学研究(英文版),2021,第1期
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