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.
This map shows the geographic impact of N. Grevesse'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 N. Grevesse with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites N. Grevesse more than expected).
This network shows the impact of papers produced by N. Grevesse. 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 N. Grevesse. The network helps show where N. Grevesse may publish in the future.
Co-authorship network of co-authors of N. Grevesse
This figure shows the co-authorship network connecting the top 25 collaborators of N. Grevesse.
A scholar is included among the top collaborators of N. Grevesse 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 N. Grevesse. N. Grevesse is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Asplund, M., A. M. Amarsi, & N. Grevesse. (2021). The chemical make-up of the Sun: A 2020 vision. Springer Link (Chiba Institute of Technology).351 indexed citations breakdown →
Grevesse, N., Pat Scott, M. Asplund, & A. J. Sauval. (2014). The elemental composition of the Sun. Astronomy and Astrophysics. 573. A27–A27.138 indexed citations
8.
Scott, Pat, N. Grevesse, M. Asplund, et al.. (2014). The elemental composition of the Sun. Astronomy and Astrophysics. 573. A25–A25.148 indexed citations
9.
Scott, Pat, M. Asplund, N. Grevesse, M. Bergemann, & A. J. Sauval. (2014). The elemental composition of the Sun. Astronomy and Astrophysics. 573. A26–A26.188 indexed citations
Asplund, M., N. Grevesse, A. J. Sauval, C. Allende Prieto, & R. Blomme. (2005). Line formation in solar granulation. Astronomy and Astrophysics. 431(2). 693–705.113 indexed citations
13.
Asplund, M., N. Grevesse, A. J. Sauval, C. Allende Prieto, & D. Kiselman. (2005). Line formation in solar granulation. Astronomy and Astrophysics. 435(1). 339–340.19 indexed citations
14.
Miglio, A., et al.. (2004). SOLAR MODEL WITH CNO REVISED ABUNDANCES. ESASP. 559. 574.3 indexed citations
15.
Asplund, M., N. Grevesse, A. J. Sauval, C. Allende Prieto, & D. Kiselman. (2004). Line formation in solar granulation. Astronomy and Astrophysics. 417(2). 751–768.467 indexed citations breakdown →
16.
Grevesse, N., A. J. Sauval, & R. Blomme. (1994). Solar Abundances of C; N; O. 154. 539.1 indexed citations
17.
Grevesse, N. & A. J. Sauval. (1992). Molecular data from solar spectroscopy. 23. 71–77.1 indexed citations
18.
Biémont, Émile, et al.. (1982). Radiative lifetimes for Pd I and the solar abundance of palladium. A&A. 108(1). 127–129.2 indexed citations
19.
Zimmermann, P., et al.. (1982). New lifetime measurements for Nb I and Rh I and the solar photospheric abundances of Nb and Rh.. A&A. 112. 337–340.1 indexed citations
20.
Grevesse, N., et al.. (1979). The elements and their isotopes in the universe; International Conference on Astrophysics, 22nd, Liege, Belgium, June 20-22, 1978, Reports. 22.1 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.