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.
Global Distribution of Neutrons from Mars: Results from Mars Odyssey
2002425 citationsW. C. Feldman, W. V. Boynton et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by T. H. Prettyman
Since
Specialization
Citations
This map shows the geographic impact of T. H. Prettyman'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 T. H. Prettyman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. H. Prettyman more than expected).
This network shows the impact of papers produced by T. H. Prettyman. 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 T. H. Prettyman. The network helps show where T. H. Prettyman may publish in the future.
Co-authorship network of co-authors of T. H. Prettyman
This figure shows the co-authorship network connecting the top 25 collaborators of T. H. Prettyman.
A scholar is included among the top collaborators of T. H. Prettyman 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 T. H. Prettyman. T. H. Prettyman is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Landis, M. E., Julie Castillo‐Rogez, P. O. Hayne, et al.. (2020). The Science Case for a Themis Asteroid Family Mission. LPI. 1640.1 indexed citations
5.
Thangjam, G., A. Nathues, K. Mengel, et al.. (2018). Is Dwarf Planet Ceres an Organic Rich Planetary Body. LPI. 2025.1 indexed citations
6.
Prettyman, T. H., Nobuyoshi Yamashita, E. Ammannito, et al.. (2018). Carbon on Ceres: Implications for Origins and Interior Evolution. Lunar and Planetary Science Conference. 1151.3 indexed citations
7.
Schörghofer, Norbert, Shane Byrne, M. E. Landis, et al.. (2017). The Putative Cerean Exosphere. The Astrophysical Journal. 850(1). 85–85.16 indexed citations
8.
Russell, C. T., C. A. Raymond, A. Nathues, et al.. (2015). First Results of the Exploration of Ceres by Dawn. 29. 2221738.1 indexed citations
9.
Raymond, C. A., S. Diniega, & T. H. Prettyman. (2015). Pandora - Discovering the origin of the moons of Mars (a proposed Discovery mission). AGU Fall Meeting Abstracts. 2015.1 indexed citations
10.
Prettyman, T. H., S. Diniega, & C. A. Raymond. (2014). PANDORA - Unlocking the mysteries of the Moons of Mars. DPS.2 indexed citations
11.
Toplis, Michael J., H. Mizzon, O. Forni, et al.. (2012). Chondritic Models of 4 Vesta: Comparison of Predicted Internal Structure and Surface Composition/Mineralogy with Data from the Dawn Mission. 2152.2 indexed citations
12.
Russell, C.T., C. A. Raymond, R. Jaumann, et al.. (2012). Dawn Completes its Mission at 4 Vesta and Prepares for 1 Ceres. elib (German Aerospace Center). 1667. 6085.1 indexed citations
13.
Prettyman, T. H., H. Y. McSween, C. A. Raymond, et al.. (2010). Dawn's GRaND to Reveal the Complex Geochemistry of Vesta. Lunar and Planetary Science Conference. 2299.1 indexed citations
14.
Feldman, W. C., T. H. Prettyman, S. Maurice, et al.. (2005). Topographic Control of Hydrogen Deposits at Mid- to Low Latitudes of Mars. 36th Annual Lunar and Planetary Science Conference. 1328.2 indexed citations
15.
Boynton, W. V., T. H. Prettyman, G. J. Taylor, et al.. (2003). Constraints on the Distribution of Hydrogen in the Polar Regions of Mars and Implications for Ice Formation Processes. AGUFM. 2003.3 indexed citations
16.
Prettyman, T. H., W. C. Feldman, W. V. Boynton, & G.W. McKinney. (2002). Analysis of Mars Odyssey Fast Neutron Data to Constrain the Hydrogen Abundance and Stratigraphy Near the South Pole. AGU Fall Meeting Abstracts. 2002.2 indexed citations
17.
Lucey, P. G., D. J. Lawrence, W. C. Feldman, et al.. (2002). A New Rock Type Found at Tycho. Lunar and Planetary Science Conference. 1056.2 indexed citations
18.
Boynton, W. V., et al.. (2002). Subsurface Ice Content in the Polar Region of Mars: Comparison Between North and South. AGU Fall Meeting Abstracts. 2002.3 indexed citations
19.
Prettyman, T. H., C.E. Moss, K. D. Ianakiev, et al.. (1998). Multielement CdZnTe detectors for high-efficiency, ambient-temperature gamma-ray spectroscopy. Transactions of the American Nuclear Society. 79. 108–109.1 indexed citations
20.
Feldman, W. C., et al.. (1996). The Lunar Prospector Gamma-Ray Spectrometer. Lunar and Planetary Science Conference. 27. 355.4 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.