Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
A test of general relativity using radio links with the Cassini spacecraft
20031.2k citationsB. Bertotti, L. Iess et al.Natureprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of B. Bertotti'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 B. Bertotti with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Bertotti more than expected).
This network shows the impact of papers produced by B. Bertotti. 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 B. Bertotti. The network helps show where B. Bertotti may publish in the future.
Co-authorship network of co-authors of B. Bertotti
This figure shows the co-authorship network connecting the top 25 collaborators of B. Bertotti.
A scholar is included among the top collaborators of B. Bertotti 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 B. Bertotti. B. Bertotti 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.
Bender, Peter, et al.. (2008). Investigation of the lunar interior with a microwave interferometer. 37. 868.1 indexed citations
2.
Iess, L., et al.. (2007). The Determination Of Titan'S Rotational State From Cassini Sar Images. AGUFM. 2007.1 indexed citations
3.
Bertotti, B., L. Iess, & Paolo Tortora. (2003). A test of general relativity using radio links with the Cassini spacecraft. Nature. 425(6956). 374–376.1211 indexed citations breakdown →
Bertotti, B., et al.. (1990). Modern Cosmology in Retrospect. Cambridge University Press eBooks. 446.3 indexed citations
6.
Bertotti, B.. (1989). Relativistic effects on earth satellites and their measurement. 42–48.1 indexed citations
7.
Ashby, Neil & B. Bertotti. (1986). Relativistic effects in local inertial frames. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 34(8). 2246–2259.44 indexed citations
Bertotti, B., et al.. (1983). Contributed papers : 10th International Conference on General Relativity and Gravitation, Padua, 4-9 July, 1983.1 indexed citations
11.
Iess, L., B. Bertotti, & M. Dobrowolny. (1983). Plasma effects on Doppler measurements of interplanetary spacecraft. I - Discontinuities and waves. IRIS Research product catalog (Sapienza University of Rome). 121(2). 203–210.1 indexed citations
Bertotti, B.. (1966). The luminosity of distant galaxies. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 294(1437). 195–207.50 indexed citations
18.
Bertotti, B.. (1964). Boundary layer problems in plasma physics. 234.
Bertotti, B.. (1956). On gravitational motion. Il Nuovo Cimento. 4(4). 898–906.66 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.