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Fan Yang1,2,3,Wei Wang2,3,Xing Wei1,Hui Zhang4,Ji-Lin Zhou4,Su-Su Shan2,3,Jie Zheng2,Wei-Kai Zong1,Ming Yang4,Yu Bai2,Song Wang2,Jia-Chen Zheng1,Yu-Ru Xu1,Yu-Feng Li1,You-Jun Lu2,3,Ji-Feng Liu2,3(Department of AstronomyBeijing Normal University;Key Laboratory of Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences;School of Astronomy and Space ScienceNanjing University).Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian[J].Research in Astronomy and Astrophysics,2022,第5期
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Noam Soker(Department of Physics,Technion).A Common Envelope Jets Supernova (CEJSN) Impostor Scenario for Fast Blue Optical Transients[J].Research in Astronomy and Astrophysics,2022,第5期
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Jaikhomba Singha1,S.Mullai Vaneshwar2,Ankit Kumar1(Department of PhysicsIndian Institute of Technology Roorkee;Department of PhysicsNational Institute of Technology Calicut).Constraining the Parameterized Neutron Star Equation of State with Astronomical Observations[J].Research in Astronomy and Astrophysics,2022,第5期
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Atila Poro1,M.G.Blackford2,S.Ranjbar Salehian3,E.Jahangiri3,M.Samiei Dastjerdi3,M.Gozarandi3,R.Karimi3,4,T.Madayen5,E.Bakhshi3,6,F.Hedayati3(Astronomy Department of the Raderon Lab.BCBurnabyCanadaastronomydep@raderonlab.ca;Variable Stars South (VSS)Congarinni ObservatoryCongarinniNSW2447;Binary Systems of South and North (BSN) ProjectContact Systems Department;Department of PhysicsKharazmi UniversityTehran;Astronomy and Astrophysics DepartmentUniversity of TorontoToronto;Department of PhysicsInstitute for Advanced Studies in Basic Sciences (IASBS)Zanjan).The First Photometric Study of AH Mic Contact Binary System[J].Research in Astronomy and Astrophysics,2022,第5期
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Marcin Wesołowski(College of Natural SciencesInstitute of PhysicsUniversity of RzeszówPigonia 1 Street35-310 Rzeszów;mwesolowski@ur.edu.pl).The Evolution of the Nucleus Surface in the Context of the Change in the Brightness of a Comet[J].Research in Astronomy and Astrophysics,2022,第5期
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Jibrin Adejoh Alhassan1,Ogbonnaya Okike2,Augustine Ejikeme Chukwude1(Department of Physics and AstronomyUniversity of Nigeria;Department of Industrial PhysicsEbonyi State University).Testing the Empirical Relationship between Forbush Decreases and Cosmic Ray Diurnal Anisotropy[J].Research in Astronomy and Astrophysics,2022,第5期
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M.F.Yıldırım(Çanakkale Onsekiz Mart UniversityAstrophysics Research Center and Ulupınar Observatory17020Çanakkale;Çanakkale Onsekiz Mart UniversityDepartment of Electricity and EnergyÇan Vocational School17400Çanakkale).Photometric Investigation of Contact Binary DY Cet Based on TESS Data[J].Research in Astronomy and Astrophysics,2022,第5期
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Alberto K.Mathias1,Sunil D.Maharaj2,Jefta M.Sunzu1,Jason M.Mkenyeleye1(Department of Mathematics and StatisticsThe University of DodomaP.O.Box 338Dodoma;Astrophysics Research CentreSchool of MathematicsStatistics and Computer ScienceUniversity of KwaZulu-NatalDurban 4000).Embedding in Anisotropic Spheres[J].Research in Astronomy and Astrophysics,2022,第4期
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Xin Pei1,2,3,Na Wang1,Dan Werthimer4,Xue-Feng Duan1,3,Jian Li1,3,Toktonur Ergesh1,3,Qi Liu1,3,Ming-Hui Cai1,3(Xinjiang Astronomical ObservatoryChinese Academy of Sciences;University of Chinese Academy of Sciences;Xinjiang Key Laboratory of Microwave Technology;Department of AstronomyUniversity of CaliforniaBerkeleyCA 94720).Design of RFSoC-based Digital Phased Array Feed (PAF) and Hybrid Architecture Beamforming System[J].Research in Astronomy and Astrophysics,2022,第4期
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Tao-Ran Li1,Xiao-Jun Jiang1,2(Key Laboratory of Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences;University of Chinese Academy of Sciences).Wind Environment Analysis of Ground-based Optical Observatory[J].Research in Astronomy and Astrophysics,2022,第4期
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Lin Wang1,2,Ye-Zhao Yu1,3,Feifei Kou4,Kuo Liu5,Xinxin Wang6,Bo Peng1(Chinapb@bao.ac.cn;Chinayuyezhao@foxmail.com;School of Astronomy and Space ScienceUniversity of Chinese Academy of SciencesBeijing;Max-Plank-Institut für RadioastronomieAuf dem Hügel 69BonnD-53121;Xinjiang Astronomical ObservatoriesChinese Academy of SciencesUrumqi;United World College of Changshu ChinaChangshu).The Study of Unusual Emission from PSR B1859+07 using FAST[J].Research in Astronomy and Astrophysics,2022,第4期
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Dong-Ming Mao1,2,Wen-Fei Yu1,Ju-Jia Zhang3,4,Zhen Yan1,Stefano Rapisarda1,Xiao-Feng Wang5,6,Jin-Ming Bai3,4(Shanghai Astronomical ObservatoryChinese Academy of Sciences;University of Chinese Academy of Sciences;Yunnan ObservatoriesChinese Academy of Sciences;Key Laboratory for the Structure and Evolution of Celestial ObjectsCAS;Physics DepartmentTsinghua University;Beijing PlanetariumBeijing Academy of Sciences and Technology).Optical and X-Ray Observations of MAXI J1820+070 During the Early Outburst Phase in 2018:Zooming in the Low Frequency QPOs[J].Research in Astronomy and Astrophysics,2022,第4期
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Zhuo-Li Yu,Xiao-Jie Xu,Xiang-Dong Li(School of Astronomy and Space Science and Key Laboratory of Modern Astronomy and AstrophysicsNanjing UniversityNanjing;xuxj@nju.edu.cn).A Study on White Dwarf Masses in Cataclysmic Variables Based on XMM-Newton and Suzaku Observations[J].Research in Astronomy and Astrophysics,2022,第4期
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S.X.Wang1,2,J.J.Zang3,1,W.Jiang1,S.J.Lei1,2,C.N.Luo1,2,Z.L.Xu1,2,J.Chang1,2(Key Laboratory of Dark Matter and Space AstronomyPurple Mountain ObservatoryChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Science and Technology of China;School of Physics and Electronic EngineeringLinyi University).A Study on Monte Carlo Simulation of the Radiation Environment above GeV at the DAMPE Orbit[J].Research in Astronomy and Astrophysics,2022,第4期
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Shu-Guang Wu,Yang Zhang(Department of AstronomyKey Laboratory for Researches in Galaxies and CosmologyUniversity of Science and Technology of China).The Nonlinear Field Equation of the Three-point Correlation Function of Galaxies:to the Second Order of Density Perturbation[J].Research in Astronomy and Astrophysics,2022,第4期
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Lin-Li Yan1,2,3,Ming-Yu Ge4,You-Li Tuo4,Ling-jun Wang4,Qing-yong Zhou5(School of Mathematics and PhysicsAnhui Jianzhu UniversityHefei;Key Laboratory of Architectural Acoustics Environment of Anhui High Education InstitutesHefei;Key Laboratory of Advanced Electronic Materials and DevicesAnhui Jianzhu UniversityHefei;Key Laboratory of Particle AstrophysicsInstitute of High Energy PhysicsChinese Academy of Sciences;State Key Laboratory of Geographic Information EngineeringXi’an Institute of Surveying and Mapping).The Time and Energy Dependence of the Vela Pulsar’s Pulse Profile in γ-Ray[J].Research in Astronomy and Astrophysics,2022,第4期
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Jiang Huang1,2,3,Wei Zhong1,2,3,Cong Yu1,2,3(School of Physics and AstronomySun Yat-Sen University;CSST Science Center for the Guangdong-Hong Kong-Macau Greater Bay Area;State Key Laboratory of Lunar and Planetary SciencesMacau University of Science and TechnologyMacau).Effects of Self-gravity on Mass-loss of the Post-impact Super-Earths[J].Research in Astronomy and Astrophysics,2022,第4期
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Chun-Xue Li1,2,Hong-Chi Wang1,2,Yue-Hui Ma1,Miao-Miao Zhang1,Chong Li3,4,Yu-Qing Zheng1(Purple Mountain Observatory and Key Laboratory of Radio AstronomyChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Science and Technology of China;School of Astronomy and Space ScienceNanjing University;Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University)Ministry of Education).Molecular Clouds Associated with HII Regions and Candidates within l=106°.65 to 109°.50 and b=-1°.85 to 0°.95[J].Research in Astronomy and Astrophysics,2022,第4期
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Maichang Lei1,Yuan Zheng1,Jianfu Zhang2,Jiancheng Wang3(College of Physics and Engineering TechnologyXingyi Normal University for Nationalities;Department of PhysicsXiangtan University;Yunnan ObservatoriesChinese Academy of Sciences).Explaining the Multiwavelength Emission of Hard-TeV BL Lac Objects Using a Truncated Conical Jet Model[J].Research in Astronomy and Astrophysics,2022,第4期
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Qing-Wen Deng1,2,Feng Wang1,2,Hui Deng1,2,Ying Mei1,2,Jing Li1,2,Oleg Smirnov3,Shao-Guang Guo4(Center for AstrophysicsSchool of Physics and Materials ScienceGuangzhou UniversityGuangzhou 51006;Great Bay CenterNational Astronomical Data CenterGuangzhou;Department of Physics and ElectronicsRhodes UniversityPO Box 94Makhanda6140;Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai).Performance Evaluation of Baseline-dependent Averaging Based on Full-scale SKA1-LOW Simulation[J].Research in Astronomy and Astrophysics,2022,第4期
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Yi Cao,Si-Dan Zhao,Xing-Yu Zhu,Hai-Chao Yu,Yi-Wei Wang,Xue-Guang Zhang(chool of Physics and TechnologyNanjing Normal University;xgzhang@njnu.edu.cn).SDSS J1042-0018:a Broad Line AGN but Misclassified as an HII Galaxy in the BPT Diagram by Flux Ratios of Narrow Emission Lines[J].Research in Astronomy and Astrophysics,2022,第4期
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Mahmoud Mohery1,Hussein M.Farid2,Alaa Ali2,3(Dept.of PhysCollege of ScienceUniversity of JeddahJeddah;AstronomySpace Science &Meteorology DepartmentFaculty of ScienceCairo UniversityGiza 12613;Astronomy Dept.Faculty of ScienceKing Abdulaziz University21589 Jeddah).The Response of the Earth’s Lower Ionosphere to Gamma-Ray Solar Flares and their Associated X-ray[J].Research in Astronomy and Astrophysics,2022,第4期
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G.Rajani1,G.M.Sowmya2,U.Paniveni3,4,R.Srikanth4(PES College of Engineering;GSSS Institute of Engineering and Technology for WomenKRS Road;Bangalore UniversityJnanabharathi;Poornaprajna Institute of Scientific ResearchDevanahalli).Solar Supergranular Fractal Dimension Dependence on the Solar Cycle Phase[J].Research in Astronomy and Astrophysics,2022,第4期
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Hu-Shan Xu1,2,Li-Ying Zhu1,2,3,Sarotsakulchai Thawicharat4,Soonthornthum Boonrucksar4(Yunnan ObservatoriesChinese Academy of Sciences (CAS);University of the Chinese Academy of Sciences;Key Laboratory of the Structure and Evolution of Celestial ObjectsChinese Academy of Sciences;National Astronomical Research Institute of).V0644 Ser:An Active Ultrashort Period Contact Binary Star[J].Research in Astronomy and Astrophysics,2022,第3期
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Huiyan Zhang1,Yong Yu2,3,Dan Yan4,Kai Tang2,Rongchuan Qiao5(School of MathematicsPhysics and StatisticsShanghai University of Engineering Science;Shanghai Astronomical ObservatoryChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences;School of Physics and Electronic InformationHuanggang Normal University;National Time Service CenterChinese Academy of Sciences).Precise Positions of Triton in 2010–2014 based on Gaia-DR2[J].Research in Astronomy and Astrophysics,2022,第3期
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Hayato Shimabukuro1,2,Yi Mao2,Jianrong Tan2,3(Yunnan UniversitySWIFARNo.2 North Green Lake Road;Department of AstronomyTsinghua University;Department of Physics &AstronomyUniversity of Pennsylvania209 South 33rd StreetPhiladelphiaPA 19104).Estimation of HII Bubble Size Distribution from 21cm Power Spectrum with Artificial Neural Networks[J].Research in Astronomy and Astrophysics,2022,第3期
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Ting Li1,2,Lei Liu1,3,Wei-Min Zheng1,3,4,Juan Zhang1,3(Shanghai Astronomical ObservatoryChinese Academy of Sciences;University of Chinese Academy of Sciences;Shanghai Key Laboratory of Space Navigation and Positioning Techniques;National Basic Public Science Data Center).The Precision Analysis of the Chinese VLBI Network in Probe Delay Measurement[J].Research in Astronomy and Astrophysics,2022,第3期
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Hao-Ting Dai1,2;Jing-Jing Zang3,4;Ying Wang1,2;Chuan-Ning Luo4;Yun-Long Zhang1,2;Zhi-Yong Zhang1,2;Yi-Feng Wei1,2;Li-Bo Wu1,2,5;Cheng-Ming Liu1,2;Cong Zhao1,2;Xiao-Lian Wang1,2;Zi-Zong Xu1,2;Guang-Shun Huang1,2(State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China;Department of Modern Physics, University of Science and Technology of China;School of Physics and Electronic Engineering, Linyi University;Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences;Gran Sasso Science Institute (GSSI)).Method of Separating Cosmic-Ray Positrons from Electrons in the DAMPE Experiment[J].Research in Astronomy and Astrophysics,2022,第3期
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