Publications of the Astronomical Society of Japan

Papers
(The H4-Index of Publications of the Astronomical Society of Japan is 18. 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 2020-05-01 to 2024-05-01.)
ArticleCitations
Third data release of the Hyper Suprime-Cam Subaru Strategic Program129
Cloud–cloud collisions and triggered star formation68
Time-resolved spectroscopy and photometry of M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in the Hα line during the non-white light flare50
Optical and X-ray observations of stellar flares on an active M dwarf AD Leonis with the Seimei Telescope, SCAT, NICER, and OISTER41
The Seimei telescope project and technical developments40
Precision radial velocity measurements by the forward-modeling technique in the near-infrared36
CO Multi-line Imaging of Nearby Galaxies (COMING). IX. 12CO(J = 2–1)/12CO(J = 1–0) line ratio on kiloparsec scales32
The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey31
The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release31
The origins and impact of outflow from super-Eddington flow26
Closure relations during the plateau emission of Swift GRBs and the fundamental plane22
SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation21
High-mass star formation in Orion B triggered by cloud–cloud collision: Merging molecular clouds in NGC 202420
Gaia’s detectability of black hole–main sequence star binaries formed in open clusters20
Rapid and efficient mass collection by a supersonic cloud–cloud collision as a major mechanism of high-mass star formation19
FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). VI. Dense gas and mini-starbursts in the W 43 giant molecular cloud complex18
HSC-XXL: Baryon budget of the 136 XXL groups and clusters18
Elemental abundances of M dwarfs based on high-resolution near-infrared spectra: Verification by binary systems18
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