Citations per year, relative to G. G. Williams G. G. Williams (= 1×)
peers
Ting-Yi Lu
Countries citing papers authored by G. G. Williams
Since
Specialization
Citations
This map shows the geographic impact of G. G. Williams'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 G. G. Williams with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. G. Williams more than expected).
This network shows the impact of papers produced by G. G. Williams. 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 G. G. Williams. The network helps show where G. G. Williams may publish in the future.
Co-authorship network of co-authors of G. G. Williams
This figure shows the co-authorship network connecting the top 25 collaborators of G. G. Williams.
A scholar is included among the top collaborators of G. G. Williams 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 G. G. Williams. G. G. Williams is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Graham, M. L., A. Rest, J. C. Wheeler, et al.. (2019). Discovery Frontiers of Explosive Transients: An ELT and LSST Perspective. Bulletin of the American Astronomical Society. 51(3). 339.1 indexed citations
Pietsch, W., M. Henze, V. Burwitz, et al.. (2010). M31N 1963-09c - Fourth recorded outburst of a recurrent nova in M 31 or a foreground U Gem system?. ATel. 3001. 1.2 indexed citations
7.
Pietsch, W., M. Henze, V. Burwitz, et al.. (2010). Apparent Nova in M31: M31N 2010-12b. 2582. 2.1 indexed citations
8.
Henze, M., W. Pietsch, V. Burwitz, et al.. (2010). Supersoft X-ray transient leads to the discovery of the second optical nova in a M 31 globular cluster. The astronomer's telegram. 3019. 1.
9.
Williams, G. G., et al.. (2010). Instrumentation suite at the MMT Observatory. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 7735. 773507–773507.1 indexed citations
Henze, M., W. Pietsch, V. Burwitz, et al.. (2009). M31N 1997-11k - a very fast recurrent nova in M31 or a foreground CV?. The astronomer's telegram. 2286. 1.1 indexed citations
12.
Henze, M., W. Pietsch, V. Burwitz, et al.. (2008). Confirmation of a recent optical nova candidate in M 31 and H- alpha identification of seven M 31 novae. ATel. 1602. 1.2 indexed citations
13.
Williams, G. G. & Peter Milne. (2008). GRB 070419A: early Super-LOTIS observations.. GRB Coordinates Network. 6328. 1.1 indexed citations
14.
Rau, A., V. Burwitz, S. B. Cenko, et al.. (2007). Optical Spectroscopy of the candidate nova M31N 2007-11b. Max Planck Institute for Plasma Physics. 1242. 1.1 indexed citations
15.
D’Arcangelo, Francesca, Alan P. Marscher, S. G. Jorstad, et al.. (2007). RAPID MULTIWAVEBAND POLARIZATION VARIABILITY IN THE QUASAR PKS 0420014: OPTICAL EMISSION FROM THE COMPACT RADIO JET.28 indexed citations
16.
Davis, Donald R., Brett Gladman, Robert Jedicke, & G. G. Williams. (2006). The Sub-Kilometer Asteroid Diameter Survey. DPS.2 indexed citations
17.
Davis, Donald R., Brett Gladman, Robert Jedicke, & G. G. Williams. (2004). SKADS: Sub-Kilometer Asteroid Diameter Survey. 36.1 indexed citations
18.
Dunham, David, et al.. (1991). The Sizes and Shapes of (4) Vesta, (216) Kleopatra, and (381) Myrrha From Occultations Observed During January 1991. 765. 54.1 indexed citations
Patterson, J., D. Schwartz, H. Bradt, et al.. (1982). Identification of the Bright X-ray Source 3A1148+719 with the Cataclysmic Variable YY Draconis. Bulletin of the American Astronomical Society. 14. 618.2 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.