Publications of the Astronomical Society of Japan

Papers
(The H4-Index of Publications of the Astronomical Society of Japan is 17. 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 2021-11-01 to 2025-11-01.)
ArticleCitations
Do blue galaxy-clusters have hot intracluster gas?260
Inference of magnetic field during the Dalton minimum: Case study with recorded sunspot areas61
ALMA detection of 321 GHz water maser emission in the radio galaxy NGC 105244
Measurement of the zodiacal light absolute intensity through Fraunhofer line spectroscopy of the night sky with the Hale telescope39
Photometric analysis on RZ Horologii: An evolved and active Algol with a δ Scuti component37
On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.726
Steady jet ejections from the innermost region of advection-dominated accretion flow around a black hole26
Introduction to Faraday tomography and its future prospects23
Abundances of phosphorus in bright F-G type main-sequence stars22
XRISM high-resolution spectroscopy of SS 433: Evidence of decreasing line-of-sight velocity dispersion along the jet21
A statistical approach to interpreting polarized dust emission of filamentary molecular clouds toward an estimate of 3D magnetic field structure19
Dynamical properties of mildly relativistic ejecta produced by the mass-loading of gamma-ray burst jets in dense ambient media19
12CO and 13CO observation of the low-metallicity dwarf galaxy DDO 15419
Cosmological evolution of dark matter subhaloes under tidal stripping by growing Milky Way-like galaxies19
Identifying hot subdwarf stars from photometric data using a Gaussian mixture model and graph neural network19
First detection of X-ray polarization and its short-term increase pre- and post-eclipse in the high-mass X-ray binary 4U 1700–37719
Strong ionospheric activity at the MWA site associated with plasma bubble measured by GNSS19
A global two-layer radiative transfer model for axisymmetric, shadowed protoplanetary disks17
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