Pau Amaro‐Seoane

9.5k total citations · 4 hit papers
74 papers, 3.2k citations indexed

About

Pau Amaro‐Seoane is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Instrumentation. According to data from OpenAlex, Pau Amaro‐Seoane has authored 74 papers receiving a total of 3.2k indexed citations (citations by other indexed papers that have themselves been cited), including 73 papers in Astronomy and Astrophysics, 8 papers in Atomic and Molecular Physics, and Optics and 7 papers in Instrumentation. Recurrent topics in Pau Amaro‐Seoane's work include Pulsars and Gravitational Waves Research (42 papers), Astrophysical Phenomena and Observations (40 papers) and Galaxies: Formation, Evolution, Phenomena (31 papers). Pau Amaro‐Seoane is often cited by papers focused on Pulsars and Gravitational Waves Research (42 papers), Astrophysical Phenomena and Observations (40 papers) and Galaxies: Formation, Evolution, Phenomena (31 papers). Pau Amaro‐Seoane collaborates with scholars based in Germany, Spain and China. Pau Amaro‐Seoane's co-authors include Frederic A. Rasio, Carl L. Rodriguez, Sourav Chatterjee, Carlos F. Sopuerta, Alberto Sesana, Marc Freitag, R. Schödel, Kyle Kremer, Claire S. Ye and M. Zevin and has published in prestigious journals such as Physical Review Letters, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

Pau Amaro‐Seoane

72 papers receiving 3.0k citations

Hit Papers

Science with the space-based interferome... 2007 2026 2013 2019 2017 2007 2018 2019 100 200 300 400

Peers

Pau Amaro‐Seoane
Bence Kocsis United States
C. P. L. Berry United Kingdom
Davide Gerosa United Kingdom
Elena M. Rossi Netherlands
I. Cognard France
Antoine Klein United States
Norbert Wex Germany
Tassos Fragos United States
Bence Kocsis United States
Pau Amaro‐Seoane
Citations per year, relative to Pau Amaro‐Seoane Pau Amaro‐Seoane (= 1×) peers Bence Kocsis

Countries citing papers authored by Pau Amaro‐Seoane

Since Specialization
Citations

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

Fields of papers citing papers by Pau Amaro‐Seoane

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Pau Amaro‐Seoane. 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 Pau Amaro‐Seoane. The network helps show where Pau Amaro‐Seoane may publish in the future.

Co-authorship network of co-authors of Pau Amaro‐Seoane

This figure shows the co-authorship network connecting the top 25 collaborators of Pau Amaro‐Seoane. A scholar is included among the top collaborators of Pau Amaro‐Seoane 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 Pau Amaro‐Seoane. Pau Amaro‐Seoane 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.
Amaro‐Seoane, Pau, et al.. (2025). A forest of gravitational waves in our Galactic Centre. Journal of Cosmology and Astroparticle Physics. 2025(11). 15–15. 1 indexed citations
2.
Mastrobuono-Battisti, A., et al.. (2024). Prograde and retrograde stars in nuclear cluster mergers. Astronomy and Astrophysics. 693. A22–A22. 2 indexed citations
3.
Kouwenhoven, M. B. N., et al.. (2023). Analysis of Kozai cycles in equal-mass hierarchical triple supermassive black hole mergers in the presence of a stellar cluster. Monthly Notices of the Royal Astronomical Society. 527(4). 10705–10725. 1 indexed citations
4.
Amaro‐Seoane, Pau. (2023). Transient Stellar Collisions as Multimessenger Probes: Nonthermal, Gravitational-wave Emission and the Cosmic Ladder Argument. The Astrophysical Journal. 947(1). 8–8. 12 indexed citations
5.
Vázquez-Aceves, Verónica, Lorenz Zwick, Elisa Bortolas, et al.. (2022). Revised event rates for extreme and extremely large mass-ratio inspirals. BOA (University of Milano-Bicocca). 15 indexed citations
6.
Rodriguez, Carl L., Scott Coughlin, Pau Amaro‐Seoane, et al.. (2022). Modeling Dense Star Clusters in the Milky Way and beyond with the Cluster Monte Carlo Code. The Astrophysical Journal Supplement Series. 258(2). 22–22. 72 indexed citations
7.
Zwick, Lorenz, Pedro R. Capelo, Elisa Bortolas, et al.. (2021). Improved gravitational radiation time-scales II: Spin–orbit contributions and environmental perturbations. Monthly Notices of the Royal Astronomical Society. 506(1). 1007–1018. 19 indexed citations
8.
Zwick, Lorenz, Pedro R. Capelo, Elisa Bortolas, Lucio Mayer, & Pau Amaro‐Seoane. (2020). Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources. Monthly Notices of the Royal Astronomical Society. 495(2). 2321–2331. 26 indexed citations
9.
Rodriguez, Carl L., M. Zevin, Pau Amaro‐Seoane, et al.. (2019). Black holes: The next generation—repeated mergers in dense star clusters and their gravitational-wave properties. Physical review. D. 100(4). 212 indexed citations breakdown →
10.
Zhang, Yu‐Peng, Shao-Wen Wei, Pau Amaro‐Seoane, Jie Yang, & Yu-Xiao Liu. (2019). Motion deviation of test body induced by spin and cosmological constant in extreme mass ratio inspiral binary system. The European Physical Journal C. 79(10). 13 indexed citations
11.
Rastello, Sara, Pau Amaro‐Seoane, Manuel Arca Sedda, et al.. (2018). Stellar black hole binary mergers in open clusters. Monthly Notices of the Royal Astronomical Society. 483(1). 1233–1246. 47 indexed citations
12.
Rodriguez, Carl L., Pau Amaro‐Seoane, Sourav Chatterjee, & Frederic A. Rasio. (2018). Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers. Physical Review Letters. 120(15). 151101–151101. 229 indexed citations breakdown →
13.
Baumgardt, Holger, Pau Amaro‐Seoane, & R. Schödel. (2017). The distribution of stars around the Milky Way’s central black hole. Springer Link (Chiba Institute of Technology). 59 indexed citations
14.
Schödel, R., E. Gallego-Cano, H. Dong, et al.. (2017). The distribution of stars around the Milky Way’s central black hole. Astronomy and Astrophysics. 609. A27–A27. 90 indexed citations
15.
Amaro‐Seoane, Pau, et al.. (2016). Retrograde binaries of massive black holes in circumbinary accretion discs. Springer Link (Chiba Institute of Technology). 6 indexed citations
16.
Brem, P., Jorge Cuadra, Pau Amaro‐Seoane, & S. Komossa. (2016). Tidal disruptions in circumbinary disks. II: Observational signatures in the reverberation spectra. 1 indexed citations
17.
Cuadra, Jorge, et al.. (2015). Infalling clouds on to supermassive black hole binaries – I. Formation of discs, accretion and gas dynamics. Monthly Notices of the Royal Astronomical Society. 455(2). 1989–2003. 25 indexed citations
18.
Roedig, C., et al.. (2012). Evolution of binary black holes in self gravitating discs. Springer Link (Chiba Institute of Technology). 73 indexed citations
19.
Amaro‐Seoane, Pau, J. R. Gair, Marc Freitag, et al.. (2007). Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals. arXiv (Cornell University). 15 indexed citations
20.
Spurzem, Rainer, Peter Berczik, G. Hensler, et al.. (2004). Physical Processes in Star–Gas Systems. Publications of the Astronomical Society of Australia. 21(2). 188–191. 5 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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