Citations per year, relative to D. A. Graham D. A. Graham (= 1×)
peers
J. F. Dolan
Countries citing papers authored by D. A. Graham
Since
Specialization
Citations
This map shows the geographic impact of D. A. Graham'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 D. A. Graham with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. A. Graham more than expected).
This network shows the impact of papers produced by D. A. Graham. 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 D. A. Graham. The network helps show where D. A. Graham may publish in the future.
Co-authorship network of co-authors of D. A. Graham
This figure shows the co-authorship network connecting the top 25 collaborators of D. A. Graham.
A scholar is included among the top collaborators of D. A. Graham 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 D. A. Graham. D. A. Graham is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Alef, W., G. Tuccari, S. Buttaccio, et al.. (2013). DBBC3: VLBI at 32 Gbits per second. Chalmers Publication Library (Chalmers University of Technology).1 indexed citations
Tuccari, G., Alessandra Bertarini, S. Buttaccio, et al.. (2010). DBBC2 Backend: Status and Development Plan. Information Visualization. 392–395.5 indexed citations
5.
Bartel, N., M. F. Bietenholz, M. P. Rupen, et al.. (1999). Expansion of Supernova 1993J. 194.1 indexed citations
6.
Pauliny‐Toth, I. I. K., et al.. (1996). The injector and variability of the quasar 3C 345. Astronomy Letters. 22(1). 14–23.2 indexed citations
7.
Seiradakis, J. H., D. A. Graham, A. Jessner, et al.. (1995). Pulsar profiles at high frequencies. I. The data.. 111. 205.1 indexed citations
8.
Rupen, M. P., J. E. Conway, A. J. Beasley, et al.. (1994). VLBI Observations of Supernova 1993J in M81: Shape, Expansion, and Distance. 103.
9.
Krichbaum, T. P., A. Witzel, D. A. Graham, C. J. Schalinski, & J. A. Zensus. (1993). New results from VLBI at 43 GHz. 181.2 indexed citations
10.
Graham, D. A., et al.. (1992). The structure of the quasar 3C-345. 18(6). 379–391.1 indexed citations
11.
Baudry, A., P. J. Diamond, R. S. Booth, D. A. Graham, & C. M. Walmsley. (1988). First VLBI synthesis observations of the excited-state OH emission sources at 4765 MHz in W3 (OH).. 201(1). 105–112.3 indexed citations
Winnberg, A., D. A. Graham, C. M. Walmsley, & R. S. Booth. (1981). A new 1720 MHz OH outburst in V1057 Cyg.. A&A. 93. 79–84.
14.
Altenhoff, W. J., et al.. (1981). Test measurements at 9 mm wavelength from the secondary focus. STIN. 83. 23504.1 indexed citations
15.
Morris, David J., D. A. Graham, W. Sieber, N. Bartel, & P. Thomasson. (1981). Observations of the polarization of average pulsar profiles at high frequency.. Astronomy & Astrophysics Supplement Series. 46. 421–472.4 indexed citations
16.
Graham, D. A., et al.. (1981). Depolarisation of pulsar integrated pulse profiles.. 100. 107–112.1 indexed citations
17.
Bartel, N., W. Sieber, & D. A. Graham. (1980). The millisecond intensity variation in the emission of radio pulsars .. 87. 282–291.3 indexed citations
18.
Morris, D., D. A. Graham, J. H. Seiradakis, et al.. (1979). Intrinsic position angles of polarization for 40 pulsars.. 73. 46–53.
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.