This map shows the geographic impact of E. A. Boldt'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 E. A. Boldt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. A. Boldt more than expected).
This network shows the impact of papers produced by E. A. Boldt. 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 E. A. Boldt. The network helps show where E. A. Boldt may publish in the future.
Co-authorship network of co-authors of E. A. Boldt
This figure shows the co-authorship network connecting the top 25 collaborators of E. A. Boldt.
A scholar is included among the top collaborators of E. A. Boldt 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 E. A. Boldt. E. A. Boldt is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
White, N. E., R. Petre, E. A. Boldt, et al.. (1995). The Next Generation X-ray Observatory for Spectroscopy. American Astronomical Society Meeting Abstracts. 187.1 indexed citations
Jahoda, K., R. F. Mushotzky, E. A. Boldt, & O. Lahav. (1991). Cross-correlation of the X-ray background with nearby galaxies. UCL Discovery (University College London). 23. 932.4 indexed citations
5.
Marshall, F. E., E. A. Boldt, S. S. Holt, et al.. (1987). X-ray Spectrometers for Observing SN1987a. Bulletin of the American Astronomical Society. 19. 735.
White, N. E., R. H. Becker, S. S. Holt, et al.. (1979). Discovery of X-Ray Emission Lines from σ Cr B with the EINSTEIN Observatory.. Bulletin of the American Astronomical Society. 11. 782.1 indexed citations
8.
Shafer, R. A., et al.. (1979). Surface Brightness Maps of the Hard X-ray Sky. Bulletin of the American Astronomical Society. 11. 442.
9.
Rothschild, R. E., E. A. Boldt, S. Holt, et al.. (1978). The cosmic X-ray experiment aboard HEAO-1. NASA STI/Recon Technical Report N. 4. 269–301.6 indexed citations
10.
Marshall, F. E., R. F. Mushotzky, E. A. Boldt, S. S. Holt, & P. J. Serlemitsos. (1978). X-Ray Emission from SS 433. IAUC. 3314. 2.1 indexed citations
11.
Marshall, F. E., E. A. Boldt, S. S. Holt, et al.. (1978). New Hard X-Ray Sources Seen by HEAO-A2. Bulletin of the American Astronomical Society. 10. 433.1 indexed citations
12.
Kaluzienski, L. J., S. S. Holt, J. H. Swank, E. A. Boldt, & P. J. Serlemitsos. (1977). X-Ray Observations of the Transient Sources H1743-32 and H1705-25 (Nova Ophiuchi 1977).. Bulletin of the American Astronomical Society. 9. 592.2 indexed citations
13.
Pravdo, S. H., R. H. Becker, E. A. Boldt, et al.. (1976). X-ray Spectra of Hercules X-1.. Bulletin of the American Astronomical Society. 8. 512.2 indexed citations
14.
Kaluzienski, L. J., S. S. Holt, E. A. Boldt, & P. J. Serlemitsos. (1976). Long-Term Variability of Cir X-1 and Aql X-1 as Observed by the Ariel-5 All-Sky Monitor.. Bulletin of the American Astronomical Society. 8. 541.1 indexed citations
Rothschild, R. E., et al.. (1974). Temporal and Spectral Studies of Her X-1, Cyg X-1, and Cyg X-3. Bulletin of the American Astronomical Society. 6. 277.
19.
Boldt, E. A., S. S. Holt, R. E. Rothschild, & P. J. Serlemitsos. (1974). What is special about Cygnus X-1?. NASA STI Repository (National Aeronautics and Space Administration). 75. 12862.1 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.