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.
Age of Jupiter inferred from the distinct genetics and formation times of meteorites
2017437 citationsT. S. Kruijer, Christoph Burkhardt et al.Proceedings of the National Academy of Sciencesprofile →
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. Budde'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. Budde with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Budde more than expected).
This network shows the impact of papers produced by G. Budde. 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. Budde. The network helps show where G. Budde may publish in the future.
Co-authorship network of co-authors of G. Budde
This figure shows the co-authorship network connecting the top 25 collaborators of G. Budde.
A scholar is included among the top collaborators of G. Budde 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. Budde. G. Budde is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Burkhardt, Christoph, et al.. (2020). Isotopic Evolution of the Protoplanetary Disk as Recorded in Mo Isotopes of Iron Meteorites. LPI. 3040.1 indexed citations
10.
Budde, G., et al.. (2020). Tungsten and Molybdenum Isotopic Constraints on the Age and Origin of CH and CB Chondrites. LPI. 2445.1 indexed citations
Tissot, François, Christoph Burkhardt, G. Budde, & T. Kleine. (2019). Multi-Elemental and Isotopic Characterization of Coarse-Grained Allende CAIs. LPI. 3136.1 indexed citations
Budde, G., Christoph Burkhardt, & T. Kleine. (2018). Early Solar System Dynamics Inferred from Molybdenum Isotope Anomalies in Meteorites. Lunar and Planetary Science Conference. 2353.3 indexed citations
15.
Kruijer, T. S., Christoph Burkhardt, G. Budde, & T. Kleine. (2017). Age of Jupiter inferred from the distinct genetics and formation times of meteorites. Proceedings of the National Academy of Sciences. 114(26). 6712–6716.437 indexed citations breakdown →
16.
Budde, G., Christoph Burkhardt, & T. Kleine. (2017). The Distinct Genetics of Carbonaceous and Non-Carbonaceous Meteorites Inferred from Molybdenum Isotopes. LPICo. 80. 6271.6 indexed citations
17.
Kruijer, T. S., T. Kleine, Christoph Burkhardt, & G. Budde. (2017). Dating the Formation of Jupiter through W and Mo Isotope Analyses of Meteorites. Lunar and Planetary Science Conference. 1386.3 indexed citations
Amelin, Y., Piers Koefoed, A. Bischoff, et al.. (2015). Pb Isotopic Age of ALM-A — A Feldspar-Rich Volcanic Rock from the Crust of the Ureilite Parent Body. LPICo. 78(1856). 5344.6 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.