This map shows the geographic impact of J. E. Beckman'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 J. E. Beckman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. E. Beckman more than expected).
This network shows the impact of papers produced by J. E. Beckman. 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 J. E. Beckman. The network helps show where J. E. Beckman may publish in the future.
Co-authorship network of co-authors of J. E. Beckman
This figure shows the co-authorship network connecting the top 25 collaborators of J. E. Beckman.
A scholar is included among the top collaborators of J. E. Beckman 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 J. E. Beckman. J. E. Beckman 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.
Elias–Rosa, N., S. Benetti, M. Turatto, et al.. (2008). SN 2002cv: a heavily obscured Type Ia supernova. Monthly Notices of the Royal Astronomical Society. 384(1). 107–122.32 indexed citations
2.
Pohlen, M., Peter Erwin, Ignacio Trujillo, & J. E. Beckman. (2008). PATHWAYS THROUGH AN ECLECTIC UNIVERSE.3 indexed citations
3.
Gutiérrez, L. & J. E. Beckman. (2008). The physics of the HII regions: the photoionization equilibrium in the HII regions of M51. 3. 177–188.
4.
Relaño, M., J. E. Beckman, & J. E. Dyson. (2003). Physical Scenarios for Supersonic Gas Flows Observed in H II Regions. 15. 281–283.1 indexed citations
5.
Knapen, J. H., et al.. (2001). The central KPC of starbursts and AGN : the la Palma connection : proceedings of a confernce held in Los Cancajos, la Palma, Spain, 7-11 May 2001. Astronomical Society of the Pacific eBooks.2 indexed citations
6.
Zurita, A., M. Rozas, & J. E. Beckman. (2000). Density bounded H II regions: ionization of the diffuseinterstellar and intergalactic media. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 9. 290–291.1 indexed citations
7.
Rozas, M., A. Zurita, J. E. Beckman, & Daniela Pérez. (2000). The ionized gas in the spiral galaxy NGC 3359. Astronomy and Astrophysics Supplement Series. 142(2). 259–273.17 indexed citations
8.
López‐Corredoira, M., J. E. Beckman, & E. Casuso. (1999). High-velocity clouds as dark matter in the Local Group. CERN Bulletin. 351(3). 920–924.1 indexed citations
9.
Rozas, M., et al.. (1998). Internal turbulence, viriality, and density bounding of the most luminous Hii regions in the spiral galaxy M 100. 338(1). 15–26.1 indexed citations
Rébolo, R., P. Molaro, C. Abia, & J. E. Beckman. (1988). Abundances of 9Be in a sample of highly metal-deficient dwarfs: implications for early galactic nucleosynthesis and primordial lithium. 193. 193–201.9 indexed citations
17.
Cepa, J. & J. E. Beckman. (1988). Parameter estimates for the orbits of M 32 and NGC 205 about the centre of mass of the M 31 system. 200. 21–25.1 indexed citations
18.
Vladilo, G., L. Crivellari, P. Molaro, & J. E. Beckman. (1987). Detections of diffuse interstellar bands toward the SN 1987A in the Large Magellanic Cloud.. 182(2).1 indexed citations
19.
Beckman, J. E. & J. P. Phillips. (1982). Submillimetre wave astronomy. Medical Entomology and Zoology.9 indexed citations
20.
Frost, Ray L., et al.. (1982). Limits on the. 253–259.3 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.