W. Ishibashi

1.4k total citations
33 papers, 928 citations indexed

About

W. Ishibashi is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, W. Ishibashi has authored 33 papers receiving a total of 928 indexed citations (citations by other indexed papers that have themselves been cited), including 33 papers in Astronomy and Astrophysics, 8 papers in Nuclear and High Energy Physics and 4 papers in Instrumentation. Recurrent topics in W. Ishibashi's work include Galaxies: Formation, Evolution, Phenomena (30 papers), Astrophysical Phenomena and Observations (23 papers) and Astrophysics and Star Formation Studies (11 papers). W. Ishibashi is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (30 papers), Astrophysical Phenomena and Observations (23 papers) and Astrophysics and Star Formation Studies (11 papers). W. Ishibashi collaborates with scholars based in Switzerland, United Kingdom and Italy. W. Ishibashi's co-authors include A. C. Fabian, R. Maiolino, T. J.-L. Courvoisier, Stefano Carniani, A. Marconi, Andrin Fluetsch, Giacomo Venturi, C. Cicone, Tiago Costa and Martin A. Bourne and has published in prestigious journals such as Nature, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

W. Ishibashi

31 papers receiving 879 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
W. Ishibashi Switzerland 14 898 206 184 23 22 33 928
Tiago Costa Germany 16 922 1.0× 286 1.4× 170 0.9× 13 0.6× 17 0.8× 28 982
D. Dultzin Mexico 19 1.0k 1.1× 234 1.1× 213 1.2× 23 1.0× 26 1.2× 63 1.0k
A. P. Thomson United Kingdom 15 885 1.0× 290 1.4× 211 1.1× 17 0.7× 18 0.8× 32 919
F. Duras Italy 10 890 1.0× 215 1.0× 259 1.4× 19 0.8× 15 0.7× 15 917
Michele Perna Italy 17 801 0.9× 242 1.2× 136 0.7× 16 0.7× 22 1.0× 43 843
Hai Fu United States 18 650 0.7× 228 1.1× 86 0.5× 38 1.7× 26 1.2× 36 682
George C. Privon United States 19 899 1.0× 264 1.3× 182 1.0× 37 1.6× 19 0.9× 50 940
Aleksandar M. Diamond‐Stanic United States 22 1.3k 1.4× 314 1.5× 305 1.7× 25 1.1× 24 1.1× 40 1.3k
Andrés Escala Chile 12 825 0.9× 115 0.6× 173 0.9× 34 1.5× 23 1.0× 34 876
M. Sánchez‐Portal Spain 15 841 0.9× 279 1.4× 137 0.7× 24 1.0× 15 0.7× 54 858

Countries citing papers authored by W. Ishibashi

Since Specialization
Citations

This map shows the geographic impact of W. Ishibashi'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 W. Ishibashi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. Ishibashi more than expected).

Fields of papers citing papers by W. Ishibashi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by W. Ishibashi. 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 W. Ishibashi. The network helps show where W. Ishibashi may publish in the future.

Co-authorship network of co-authors of W. Ishibashi

This figure shows the co-authorship network connecting the top 25 collaborators of W. Ishibashi. A scholar is included among the top collaborators of W. Ishibashi 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 W. Ishibashi. W. Ishibashi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Ishibashi, W.. (2024). How black hole activity may influence exoplanetary evolution in our Galaxy. Monthly Notices of the Royal Astronomical Society. 533(1). 455–463. 1 indexed citations
2.
Ishibashi, W., et al.. (2024). Gravitational wave mergers of accreting binary black holes in AGN discs. Monthly Notices of the Royal Astronomical Society. 529(2). 883–892. 4 indexed citations
3.
Ishibashi, W., A. C. Fabian, & P. C. Hewett. (2024). Are BAL outflows powered by radiation pressure on dust?. Monthly Notices of the Royal Astronomical Society. 533(4). 4384–4392. 1 indexed citations
4.
Ishibashi, W. & A. C. Fabian. (2022). What powers galactic outflows: nuclear starbursts or AGN?. Monthly Notices of the Royal Astronomical Society. 516(4). 4963–4970. 5 indexed citations
5.
Ishibashi, W. & A. C. Fabian. (2022). AGN cool feedback and analogy with X-ray binaries: from radiation pressure to cosmic ray-driven outflows. Monthly Notices of the Royal Astronomical Society. 519(2). 1931–1940. 2 indexed citations
6.
Fluetsch, Andrin, R. Maiolino, Stefano Carniani, et al.. (2021). Properties of the multiphase outflows in local (ultra)luminous infrared galaxies. Monthly Notices of the Royal Astronomical Society. 505(4). 5753–5783. 75 indexed citations
7.
Ishibashi, W., et al.. (2020). Evolution of binary black holes in AGN accretion discs: Disc-binary interaction and gravitational wave emission. Springer Link (Chiba Institute of Technology). 22 indexed citations
8.
Ishibashi, W.. (2020). AGN anisotropic radiative feedback set by black hole spin. Monthly Notices of the Royal Astronomical Society. 495(2). 2515–2523. 3 indexed citations
9.
Ishibashi, W.. (2019). AGN radiative feedback in the early growth of massive black holes. Monthly Notices of the Royal Astronomical Society. 489(4). 5225–5230. 3 indexed citations
10.
Ishibashi, W., A. C. Fabian, & C. S. Reynolds. (2019). Radiation pattern and outflow geometry: a new probe of black hole spin?. Monthly Notices of the Royal Astronomical Society. 486(2). 2210–2214. 8 indexed citations
11.
Ishibashi, W. & A. C. Fabian. (2018). Variations on a theme of AGN-driven outflows: luminosity evolution and ambient density distribution. Monthly Notices of the Royal Astronomical Society. 481(4). 4522–4531. 9 indexed citations
12.
Maiolino, R., H. R. Russell, A. C. Fabian, et al.. (2017). Star formation inside a galactic outflow. Nature. 544(7649). 202–206. 143 indexed citations
13.
Ishibashi, W., et al.. (2016). AGN–starburst evolutionary connection: a physical interpretation based on radiative feedback. Monthly Notices of the Royal Astronomical Society. 463(2). 1291–1296. 24 indexed citations
14.
Ishibashi, W. & T. J.-L. Courvoisier. (2012). The physical origin of the X-ray power spectral density break timescale in accreting black holes. Astronomy and Astrophysics. 540. L2–L2. 7 indexed citations
15.
Ishibashi, W. & A. C. Fabian. (2012). Active galactic nucleus feedback and triggering of star formation in galaxies. Monthly Notices of the Royal Astronomical Society. 427(4). 2998–3005. 109 indexed citations
16.
Ishibashi, W. & T. J.-L. Courvoisier. (2010). Synchrotron radio emission in radio-quiet AGNs. Astronomy and Astrophysics. 525. A118–A118. 13 indexed citations
17.
Ishibashi, W. & T. J.-L. Courvoisier. (2010). X-ray power law spectra in active galactic nuclei. Astronomy and Astrophysics. 512. A58–A58. 29 indexed citations
18.
Ishibashi, W. & T. J.-L. Courvoisier. (2009). X-ray variability time scales in active galactic nuclei. Springer Link (Chiba Institute of Technology). 8 indexed citations
19.
Ishibashi, W. & T. J.-L. Courvoisier. (2009). AGN UV and X-ray luminosities in clumpy accretion flows. Astronomy and Astrophysics. 495(1). 113–120. 15 indexed citations
20.
Beckmann, V., W. Ishibashi, E. Bottacini, M. Ajello, & J. Greiner. (2007). Swift and INTEGRAL observation of 1ES 1959+650. Max Planck Institute for Plasma Physics. 1317. 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.

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