This map shows the geographic impact of J. A. Tyson'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. A. Tyson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. A. Tyson more than expected).
This network shows the impact of papers produced by J. A. Tyson. 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. A. Tyson. The network helps show where J. A. Tyson may publish in the future.
Co-authorship network of co-authors of J. A. Tyson
This figure shows the co-authorship network connecting the top 25 collaborators of J. A. Tyson.
A scholar is included among the top collaborators of J. A. Tyson 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. A. Tyson. J. A. Tyson is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Zhan, Hu & J. A. Tyson. (2017). Cosmology with the Large Synoptic Survey Telescope. arXiv (Cornell University).2 indexed citations
7.
Strauss, Michael A., J. A. Tyson, Donald W. Sweeney, et al.. (2010). LSST Observatory System and Science Opportunities. 215.1 indexed citations
8.
Cook, Kem H., Philip A. Pinto, Francisco Delgado, et al.. (2009). LSST: Cadence Design and Simulation. AAS. 213.2 indexed citations
9.
Pinto, Philip A., K. H. Cook, Francisco Delgado, et al.. (2007). LSST: Cadence Design and Simulation. American Astronomical Society Meeting Abstracts. 211.2 indexed citations
10.
Pinto, Philip A., K. H. Cook, Francisco Delgado, et al.. (2006). LSST Survey Strategy: Cadence Design and Simulation. American Astronomical Society Meeting Abstracts. 209.1 indexed citations
11.
Stubbs, C. W., Donald W. Sweeney, & J. A. Tyson. (2004). An Overview of the Large Synoptic Survey Telescope (LSST) System. AAS. 205.4 indexed citations
12.
Tyson, J. A.. (2004). The Large Synoptic Survey Telescope Science Requirements. American Astronomical Society Meeting Abstracts. 205.1 indexed citations
13.
Fassnacht, C. D., et al.. (2004). Strong Lensing Studies with the LSST. American Astronomical Society Meeting Abstracts. 205.
14.
Angel, J. R. P., Charles F. Claver, H. M. Martin, et al.. (2001). LSST Optical Design. AAS. 199.1 indexed citations
15.
Tyson, J. A., et al.. (2001). The Deep Lens Survey: Overview. American Astronomical Society Meeting Abstracts. 199.1 indexed citations
16.
Tyson, J. A., P. Guhathakurta, G. M. Bernstein, & Piet Hut. (1992). Limits on the Surface Density of Faint Kuiper Belt Objects. American Astronomical Society Meeting Abstracts. 181.6 indexed citations
17.
Bernstein, G. M., J. A. Tyson, G. Efstathiou, Neal Katz, & Puragra Guhathakurta. (1991). Angular Correlations of Faint Galaxies. Bulletin of the American Astronomical Society. 23. 897.
18.
Weymann, R. J., David W. Latham, J. R. P. Angel, et al.. (1980). An Optical Three-Way Split - Triple Quasar PG1115+08. Science News. 118. 4.2 indexed citations
19.
Tyson, J. A.. (1980). A CCD Imaging Polarimeter. Bulletin of the American Astronomical Society. 12. 488.1 indexed citations
20.
Rudnick, L., William C. Saslaw, & J. A. Tyson. (1979). Radio Observations of Extended Lobes with Optical Counterparts. Bulletin of the American Astronomical Society. 11. 716.1 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.