This map shows the geographic impact of Edward Seidel'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 Edward Seidel with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Edward Seidel more than expected).
This network shows the impact of papers produced by Edward Seidel. 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 Edward Seidel. The network helps show where Edward Seidel may publish in the future.
Co-authorship network of co-authors of Edward Seidel
This figure shows the co-authorship network connecting the top 25 collaborators of Edward Seidel.
A scholar is included among the top collaborators of Edward Seidel 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 Edward Seidel. Edward Seidel is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Allen, Gabrielle, Jarosław Nabrzyski, Edward Seidel, et al.. (2009). Proceedings of the 9th International Conference on Computational Science.28 indexed citations
3.
Bondarescu, R., Gabrielle Allen, Michael Russell, et al.. (2003). The Astrophysics Simulation Collaboratory portal: A framework for effective distributed \nresearch. eScholarship (California Digital Library).13 indexed citations
4.
Benger, Werner, Hans‐Christian Hege, Thomas Radke, & Edward Seidel. (2001). Data Description Via a Generalized Fiber Bundle Data Model. Max Planck Digital Library.2 indexed citations
Alcubierre, Miguel, Bernd Brügmann, Denis Pollney, Edward Seidel, & Ryōji Takahashi. (2001). Black hole excision for dynamic black holes. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 64(6).67 indexed citations
Allen, Gabrielle, Karen Camarda, & Edward Seidel. (1998). Evolution of distorted black holes: A Perturbative approach. CERN Bulletin.1 indexed citations
11.
Camarda, Karen & Edward Seidel. (1998). Numerical evolution of dynamic 3D black holes: Extracting waves. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 57(6). R3204–R3208.12 indexed citations
Seidel, Edward, et al.. (1996). Formation of Bosonic Compact Objects. 1067.1 indexed citations
15.
Massó, Joan, et al.. (1996). A 3-D Apparent Horizon Finder. 631.2 indexed citations
16.
Brandt, Steven R. & Edward Seidel. (1996). Evolution of distorted rotating black holes. III. Initial data. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 54(2). 1403–1416.51 indexed citations
17.
Anninos, Peter, David Bernstein, Steven R. Brandt, et al.. (1995). Dynamics of Apparent and Event Horizons. Physical Review Letters. 74(5). 630–633.44 indexed citations
18.
Massó, Joan, Edward Seidel, & P. N. Walker. (1994). Adaptative Mesh Refinement in Numerical Relativity. CERN Bulletin. 634.1 indexed citations
19.
Seidel, Edward & Wai-Mo Suen. (1994). NUMERICAL RELATIVITY. International Journal of Modern Physics C. 5(2). 181–187.1 indexed citations
20.
Anninos, Peter, et al.. (1993). Visualizing black hole space-times. IEEE Computer Graphics and Applications. 13(1). 13–14.1 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.