This map shows the geographic impact of F. A. Primini'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 F. A. Primini with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. A. Primini more than expected).
This network shows the impact of papers produced by F. A. Primini. 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 F. A. Primini. The network helps show where F. A. Primini may publish in the future.
Co-authorship network of co-authors of F. A. Primini
This figure shows the co-authorship network connecting the top 25 collaborators of F. A. Primini.
A scholar is included among the top collaborators of F. A. Primini 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 F. A. Primini. F. A. Primini 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.
Evans, I. N., Juan Rafael Martínez-Galarza, Joseph B. Miller, et al.. (2024). The Chandra Source Catalog Release 2 Series. The Astrophysical Journal Supplement Series. 274(2). 22–22.17 indexed citations
2.
Barnard, R., et al.. (2013). AROUND 200 NEW X-RAY BINARY IDs FROM 13 YR OF CHANDRA OBSERVATIONS OF THE M31 CENTER. DSpace@MIT (Massachusetts Institute of Technology).10 indexed citations
3.
Garcia, Mary Lynn, et al.. (2010). Optical ID of CXOM31 J004253.1+411422, a bright Black Hole X-ray Nova in M31. ATel. 2474. 1.
4.
Stefano, R. Di, et al.. (2008). Two new supersoft X-ray sources in M31 identified as classical novae. ATel. 1672. 1.1 indexed citations
5.
Galache, J. L., M. A. P. Torres, D. Steeghs, et al.. (2006). Chandra observations of the M31 transients XMMU J004215.8+411924 and SWIFT J004217.4+411532. The astronomer's telegram. 969. 1.1 indexed citations
6.
Fruscione, Antonella, Jonathan McDowell, G. E. Allen, et al.. (2006). CIAO: Chandra's data analysis system. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 6270. 62701V–62701V.2 indexed citations
Worrall, D. M., F. K. Knight, P. L. Nolan, et al.. (1981). The hard X-ray spectrum of X Persei. The Astrophysical Journal. 247. L31–L31.7 indexed citations
16.
Nolan, P. L., D. E. Gruber, F. K. Knight, et al.. (1981). Hard X-ray spectrum of Cygnus X-l. Nature. 293(5830). 275–277.24 indexed citations
17.
Levine, Alan M., P. B. Byrne, B. A. Cooke, et al.. (1979). Preliminary Results of the HEAO A4 Hard X-ray Sky Survey (13-180 keV). Bulletin of the American Astronomical Society. 11. 429.1 indexed citations
18.
Byrne, P. B., C. A. Dobson, J. Doty, et al.. (1979). Hard X-ray Observations of a 38 sec Pulsar. Bulletin of the American Astronomical Society. 11. 424.1 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.