Keiichi Wada

3.1k total citations
70 papers, 1.6k citations indexed

About

Keiichi Wada is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, Keiichi Wada has authored 70 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 68 papers in Astronomy and Astrophysics, 9 papers in Nuclear and High Energy Physics and 6 papers in Computational Mechanics. Recurrent topics in Keiichi Wada's work include Astrophysics and Star Formation Studies (54 papers), Galaxies: Formation, Evolution, Phenomena (49 papers) and Astrophysical Phenomena and Observations (32 papers). Keiichi Wada is often cited by papers focused on Astrophysics and Star Formation Studies (54 papers), Galaxies: Formation, Evolution, Phenomena (49 papers) and Astrophysical Phenomena and Observations (32 papers). Keiichi Wada collaborates with scholars based in Japan, United States and Chile. Keiichi Wada's co-authors include Colin Norman, Jin Koda, Asao Habe, Takayuki R. Saitoh, Kohji Tomisaka, Masatoshi Imanishi, Junichiro Makino, Eiichiro Kokubo, Takashi Okamoto and Yutaka Fujita and has published in prestigious journals such as Science, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Keiichi Wada

66 papers receiving 1.6k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Keiichi Wada Japan 24 1.6k 224 217 90 58 70 1.6k
Blakesley Burkhart United States 24 1.5k 1.0× 202 0.9× 204 0.9× 84 0.9× 48 0.8× 79 1.6k
Makoto Miyoshi Japan 17 1.5k 0.9× 139 0.6× 439 2.0× 88 1.0× 48 0.8× 60 1.5k
G. Tenorio‐Tagle Mexico 27 2.2k 1.4× 281 1.3× 359 1.7× 106 1.2× 36 0.6× 130 2.3k
Mattia C. Sormani Germany 21 1.3k 0.8× 238 1.1× 170 0.8× 85 0.9× 35 0.6× 70 1.4k
E. Corbelli Italy 24 1.7k 1.1× 419 1.9× 181 0.8× 97 1.1× 18 0.3× 59 1.8k
M. Pereira-Santaella Spain 27 1.7k 1.1× 385 1.7× 234 1.1× 100 1.1× 21 0.4× 109 1.8k
Michael Y Grudić United States 23 1.4k 0.9× 300 1.3× 112 0.5× 52 0.6× 32 0.6× 56 1.5k
M. Krips France 27 2.0k 1.2× 302 1.3× 270 1.2× 123 1.4× 17 0.3× 70 2.0k
I. Valtchanov Spain 22 1.1k 0.7× 380 1.7× 192 0.9× 48 0.5× 23 0.4× 68 1.1k
Shinki Oyabu Japan 19 1.1k 0.7× 349 1.6× 179 0.8× 47 0.5× 43 0.7× 95 1.2k

Countries citing papers authored by Keiichi Wada

Since Specialization
Citations

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

Fields of papers citing papers by Keiichi Wada

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Keiichi Wada

This figure shows the co-authorship network connecting the top 25 collaborators of Keiichi Wada. A scholar is included among the top collaborators of Keiichi Wada 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 Keiichi Wada. Keiichi Wada 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
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Camps, Peter, et al.. (2024). Intrinsic line profiles for X-ray fluorescent lines in SKIRT. Astronomy and Astrophysics. 688. L33–L33.
4.
Yamada, Satoshi, Yoshihiro Ueda, T. Kawamuro, et al.. (2024). [O iv]- and [Ne v]-weak Active Galactic Nuclei Hidden by Compton-thick Material in Late Mergers. The Astrophysical Journal. 965(2). 153–153. 3 indexed citations
5.
Tanimoto, A., et al.. (2023). Circumnuclear Multiphase Gas in the Circinus Galaxy. V. The Origin of the X-Ray Polarization in the Circinus Galaxy. The Astrophysical Journal. 958(2). 150–150. 5 indexed citations
6.
Wada, Keiichi, et al.. (2023). Multiphase Gas Nature in the Sub-parsec Region of the Active Galactic Nuclei. I. Dynamical Structures of Dusty and Dust-free Outflow. The Astrophysical Journal. 950(1). 72–72. 11 indexed citations
7.
Camps, Peter, M. Baes, Frederik De Ceuster, et al.. (2023). Self-consistent dust and non-LTE line radiative transfer with SKIRT. Astronomy and Astrophysics. 678. A175–A175. 12 indexed citations
8.
Nakagawa, Takao, et al.. (2022). Probing Dynamics and Thermal Properties Inside Molecular Tori with CO Rovibrational Absorption Lines. The Astrophysical Journal. 934(1). 25–25. 7 indexed citations
9.
Büchner, Johannes, Murray Brightman, Mislav Baloković, et al.. (2021). Physically motivated X-ray obscurer models. Astronomy and Astrophysics. 651. A58–A58. 25 indexed citations
10.
Aalto, S., N. Falstad, Keiichi Wada, et al.. (2020). ALMA resolves the remarkable molecular jet and rotating wind in the extremely radio-quiet galaxy NGC 1377. Springer Link (Chiba Institute of Technology). 20 indexed citations
11.
Imanishi, Masatoshi, Kouichiro Nakanishi, Takuma Izumi, & Keiichi Wada. (2018). ALMA Reveals an Inhomogeneous Compact Rotating Dense Molecular Torus at the NGC 1068 Nucleus. The Astrophysical Journal Letters. 853(2). L25–L25. 65 indexed citations
12.
Costagliola, F., Kazushi Sakamoto, J. S. Gallagher, et al.. (2017). Luminous, pc-scale CO 6−5 emission in the obscured nucleus of NGC 1377. Astronomy and Astrophysics. 608. A22–A22. 11 indexed citations
13.
Costagliola, F., S. Müller, Kazushi Sakamoto, et al.. (2016). A precessing molecular jet signaling an obscured, growing supermassive black hole in NGC 1377?. Springer Link (Chiba Institute of Technology). 19 indexed citations
14.
Wagner, R. M., Subo Dong, T. Bensby, et al.. (2012). MOA 2012 BLG-320: Discovery and Observations of a Nova Candidate Towards the Galactic Bulge. ATel. 4157. 1. 1 indexed citations
15.
Wada, Keiichi, Eiichiro Kokubo, & Junichiro Makino. (2006). High‐Resolution Simulations of a Moon‐forming Impact and Postimpact Evolution. The Astrophysical Journal. 638(2). 1180–1186. 33 indexed citations
16.
Okuda, Koji, et al.. (2004). Nonlinear Evolution Equation of a Step with Anisotropy in a Diffusion Field for the Two-Sided Model. Journal of the Physical Society of Japan. 73(5). 1362–1370. 1 indexed citations
17.
Koda, Jin & Keiichi Wada. (2002). Intrinsic errors of the central galactic mass derived from rotation curves\n under the influence of a weak non-axisymmetric potential. Springer Link (Chiba Institute of Technology). 13 indexed citations
18.
Wada, Keiichi & Colin Norman. (2001). Numerical Models of the Multiphase Interstellar Matter with Stellar Energy Feedback on a Galactic Scale. The Astrophysical Journal. 547(1). 172–186. 142 indexed citations
19.
Wada, Keiichi & Jin Koda. (2001). Multi-Phase Gas Dynamics in a Weak Barred Potential. Publications of the Astronomical Society of Japan. 53(6). 1163–1170. 20 indexed citations
20.
Fukuda, Hiroyuki, Asao Habe, & Keiichi Wada. (2000). The Effect of the Self‐Gravity of Gas on Gas Fueling in a Barred Galaxy with a Supermassive Black Hole. The Astrophysical Journal. 529(1). 109–118. 22 indexed citations

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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