Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Upper limits on the isotropic gravitational radiation background from pulsar timing analysis
1983565 citationsG. S. Downs et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of G. S. Downs'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. S. Downs with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. S. Downs more than expected).
This network shows the impact of papers produced by G. S. Downs. 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. S. Downs. The network helps show where G. S. Downs may publish in the future.
Co-authorship network of co-authors of G. S. Downs
This figure shows the co-authorship network connecting the top 25 collaborators of G. S. Downs.
A scholar is included among the top collaborators of G. S. Downs 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. S. Downs. G. S. Downs is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Roth, L. E., G. S. Downs, R. S. Saunders, & G. Schubert. (1985). Mars: Seasonally variable radar reflectivity. NASA STI Repository (National Aeronautics and Space Administration). 559. 248–250.2 indexed citations
Downs, G. S., P. J. Mouginis‐Mark, S. H. Zisk, & T. W. Thompson. (1982). New Radar-Derived Topography for the Equatorial Belt of Mars. Lunar and Planetary Science Conference. 182–183.3 indexed citations
Roth, L. E., M. Kobrick, G. S. Downs, R. S. Saunders, & G. Schubert. (1981). Martian center of mass - center of figure offset.. 372–374.2 indexed citations
8.
Downs, G. S. & P. E. Reichley. (1980). Techniques for measuring arrival times of pulsar signals 1: DSN observations from 1968 to 1980. STIN. 80. 33317.2 indexed citations
9.
Saunders, R. S., et al.. (1980). Early volcanic-tectonic province: Coprates region of Mars.. 74–76.5 indexed citations
10.
Mouginis‐Mark, P. J., S. H. Zisk, & G. S. Downs. (1980). Characterization of Martian surface materials from earth-based radar - The Memnonia Fossae region. Lunar and Planetary Science Conference Proceedings. 1. 823.7 indexed citations
11.
Roth, L. E., G. S. Downs, R. S. Saunders, & G. Schubert. (1979). Atlas of radar topography of Mars.. 436–437.1 indexed citations
12.
Roth, L. E., G. S. Downs, R. S. Saunders, & G. Schubert. (1979). Radar morphometry of craters, basins and volcanic landforms on Mars. 71.1 indexed citations
Downs, G. S. & P. E. Reichley. (1975). Radar ranging of the planet Mars at 8495 MHz. 29. 95–106.2 indexed citations
17.
Downs, G. S.. (1974). Interplanetary navigation using pulsating radio sources. NASA STI Repository (National Aeronautics and Space Administration).56 indexed citations
Melbourne, W. G., et al.. (1970). Ephemeris, Radar Radius, and Radar Topography of Mars. Bulletin of the American Astronomical Society. 2. 211.1 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.