Yoshiaki Sofue
About
In The Last Decade
Yoshiaki Sofue
196 papers receiving 2.9k citations
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 2.9k
- Nuclear and High Energy Physics 998
- Instrumentation 443
- Spectroscopy 136
- Atomic and Molecular Physics, and Optics 126
Countries citing papers authored by Yoshiaki Sofue
This map shows the geographic impact of Yoshiaki Sofue's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Yoshiaki Sofue with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Yoshiaki Sofue more than expected).
Fields of papers citing papers by Yoshiaki Sofue
This network shows the impact of papers produced by Yoshiaki Sofue. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Yoshiaki Sofue. The network helps show where Yoshiaki Sofue may publish in the future.
Co-authorship network of co-authors of Yoshiaki Sofue
This figure shows the co-authorship network connecting the top 25 collaborators of Yoshiaki Sofue. A scholar is included among the top collaborators of Yoshiaki Sofue based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Yoshiaki Sofue. Yoshiaki Sofue is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 11 | |
| 3 | The central regions of the Galaxy and galaxies | 45 |
| 4 | ISOPHOT 175 Micron Survey in the Lockman Hole | 0 |
| 5 | Distribution and Dynamics of Molecular Gas in the Galaxy M51-1-Data and Spiral Structure | 1 |
| 6 | CO Observations of Edge-on Galaxies. IV. NGC 4565: Radial Variation of the H_{normalsize2 }-to-H{I} Ratio | 3 |
| 7 | A study of the composite supernova remnant G 18.95-1.1 | 1 |
| 8 | CO observations of the central region of the galaxy NGC 4258. | 1 |
| 9 | A study of the radio spectral index in the galactic centre region : evidence for an unusual nonthermal emission component. | 0 |
| 10 | The identification of galactic radio sources based on a comparison of radio-continuum and infrared emission | 1 |
| 11 | A 10-GHz radio continuum survey of the galactic plane region. I. A complex region at l=21°-26° | 0 |
| 12 | A Negative Search for CO Absorption Lines(J=0-1) toward High-Redshift Quasars | 0 |
| 13 | A 1.5-m Millimeter-Wave Telescope with Acousto-Optical Spectrometers at Nagoya University | 2 |
| 14 | 10-GHz Observations of the Supernova Remnant G109.1-1.0 Containing an X-Ray Pulsar〔英文〕 | 2 |
| 15 | Neutral Hydrogen in M31 - Part Three - the Warping of HI Disk | 3 |
| 16 | Neutral Hydrogen in M31 - Part Four - Comparison with Optical Data and the Star Formation Rate | 1 |
| 17 | Neutral Hydrogen in M31-1-The Distribution of H1 Gas and Spiral Arms | 4 |
| 18 | Neutral Hydrogen in M31 - Part One - the Distribution of HI Gas and Spiral Arms | 7 |
| 19 | Radio continuum observations of the North Polar Spur at 1420 MHz. | 4 |
| 20 | Radio spurs and spiral structure of the galaxy-1-Optical and radio brightness distributions in the Milky Way | 1 |
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.