Research in Astronomy and Astrophysics

Papers
(The H4-Index of Research in Astronomy and Astrophysics is 21. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2022-05-01 to 2026-05-01.)
ArticleCitations
Dreicer Electric Field Definition and Runaway Electrons in Solar Flares1004
Research on Beam Calibration Technology of Phased Array Feed134
Small-scale Clustering of Star-forming Galaxies Relative to Early-type and Late-type Galaxies: IllustrisTNG versus the Sloan Digital Sky Survey82
Modeling GRB 171205A: A Semi-analytical Approach to Shock Dynamics from Thick to Thin Media73
Photometric Calibration of Spectral Imaging CoronaGraph with Dual-wavelength Observation59
Relation between Mass and Radius of Exoplanets Distinguished by their Density58
Photometric Monitoring of Blazar 3C 66A with the Yunnan University Astronomical Observatory 1 m Telescope51
Transverse Velocity Field Measurements in High-resolution Solar Images Based on Deep Learning51
Optical and X-Ray Studies of Marginal Contact Binary RW Dor Using TESS and XMM-Newton Observatories37
Fermi Blazars in the Zwicky Transient Facility Survey: Properties of Large Optical Variations36
A Spectral Element Method to Compute Earth’s Free Core Nutation36
A Region Selection Method for Real-time Local Correlation Tracking of Solar Full-disk Magnetographs34
Chemical Tagging of Tidal Tail Star Candidates of NGC 636233
The Influence of Velocity-dependent Correction Factor on Proton Decay Reactions in Massive White Dwarfs29
The Role of Jets in Exploding Supernovae and in Shaping their Remnants28
Cosmological Constraints on Neutrino Masses in Light of JWST Red and Massive Candidate Galaxies27
O’Connell Effect and Period Variations on Solar-like Contact Binary EF Boo27
A Fast Radio Burst Backend for the Tianlai Dish Pathfinder Array26
Diagnostic Functions of Solar Coronal Magnetic Fields from Radio Observations23
Toward a Direct Measurement of the Cosmic Acceleration: The Pilot Observation of HI 21 cm Absorption Line at FAST23
A 3 Giga Sample Per Second 14-bit Digital Receiver with 9 GHz Input Bandwidth for Solar Radio Observation22
Tracklet-to-object Matching for Climbing Starlink Satellites through Recursive Orbit Determination and Prediction21
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