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.
THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS
2010631 citationsAlexander Heger, R. D. Hoffman et al.profile →
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
2002605 citationsT. Rauscher, Alexander Heger et al.The Astrophysical Journalprofile →
The r-process and neutrino-heated supernova ejecta
1994497 citationsS. E. Woosley, J. R. Wilson et al.The Astrophysical Journalprofile →
The nu-process
1990412 citationsS. E. Woosley, D. H. Hartmann et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of R. D. Hoffman'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 R. D. Hoffman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. D. Hoffman more than expected).
This network shows the impact of papers produced by R. D. Hoffman. 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 R. D. Hoffman. The network helps show where R. D. Hoffman may publish in the future.
Co-authorship network of co-authors of R. D. Hoffman
This figure shows the co-authorship network connecting the top 25 collaborators of R. D. Hoffman.
A scholar is included among the top collaborators of R. D. Hoffman 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 R. D. Hoffman. R. D. Hoffman is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Hoffman, R. D., et al.. (2010). Reaction rate sensitivity of 44Ti production in massive stars and implications of a thick target yield measurement for 40Ca(α,γ)44Ti. 240.1 indexed citations
Hoffman, R. D., Bernhard Müller, & Hans‐Thomas Janka. (2008). Nucleosynthesis in O-Ne-Mg Supernovae. The Astrophysical Journal. 676(2). L127–L130.21 indexed citations
Rauscher, T., Alexander Heger, R. D. Hoffman, & S. E. Woosley. (2000). Nucleosynthesis in massive stars revisited.7 indexed citations
10.
Heger, Alexander, R. D. Hoffman, T. Rauscher, & S. E. Woosley. (2000). Nucleosynthesis in Massive Stars - Including All Stable Isotopes. CERN Bulletin. 105.1 indexed citations
11.
Hartmann, D. H., J. Myers, S. E. Woosley, R. D. Hoffman, & W. C. Haxton. (1999). Neutrino Process Contributions to LiBeB Nucleosynthesis. ASPC. 171. 235.1 indexed citations
12.
Hartmann, D. H., P. Predehl, J. Greiner, et al.. (1997). On Flamsteed's supernova Cas A. Nuclear Physics A. 621(1-2). 83–91.18 indexed citations
Woosley, S. E., F. X. Timmes, R. D. Hoffman, et al.. (1995). Radioactivities Made in Supernovae. Annals of the New York Academy of Sciences. 759(1). 388–391.1 indexed citations
16.
Woosley, S. E., J. R. Wilson, Grant J. Mathews, R. D. Hoffman, & B. S. Meyer. (1994). The r-process and neutrino-heated supernova ejecta. The Astrophysical Journal. 433. 229–229.497 indexed citations breakdown →
Hoffman, R. D.. (1992). Structural Geology of the Concord Area. 79–89.1 indexed citations
19.
Hoffman, R. D. & S. E. Woosley. (1991). The α-Process and the ρ-Process. Bulletin of the American Astronomical Society. 23. 975.4 indexed citations
20.
Hoffman, R. D. & S. E. Woosley. (1986). Explosive Nucleosynthesis of Isotopes Important to Gamma-Line Astronomy. Bulletin of the American Astronomical Society. 18. 948.1 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.